Let ${\bf C}$ be a category, $\alpha$ an ordinal number, and $\zeta$ a function $\alpha \times \alpha \to \alpha$ (see note 1). Let us define a $5$-tuple $\zeta \ast {\bf C} := (D_o,D_h,u,v,d)$ as follows: $D_o$ is just the object class of $\bf C$, while $D_h$ is the quotient of $\coprod_{i \in \alpha} \hom({\bf C})$ by the equivalence $\mathcal R$ that amalgamates two couples $(f,i)$ and $(g,j)$ iff $f=g={\rm id}_{\bf C}(A)$ for some $A \in {\rm Ob}({\bf C})$; $u$ and $v$ are functions $D_h \to D_o$ taking the equivalence class $(f,i) \bmod \mathcal R$ to $s(f)$ and $t(f)$, respectively; and $d$ is the mapping $D_h \times_{v,u} D_h \to D_h$ sending a pair $((f,i)\bmod \mathcal R,(g,j) \bmod \mathcal R)$ to $(f,i) \bmod \mathcal R$, respectively to $(g,j) \bmod \mathcal R$, if $g$, respectively $f$, is an identity of $\bf C$, and to $(fg,\zeta(i,j)) \bmod \mathcal R$ otherwise.

It is clear that $\zeta \ast \bf C$ is itself a category: I'm using it as a toy example, while looking forward to finding something more "natural", to introduce a generalized notion of limit (and its dual) which, on the one hand, makes sense in much more abstract settings than categories (e.g., Mitchell's semicats or even Ehresmann's neocats), and on the other hand, _may perhaps_ be an effective surrogate of limits - I can't say, at present, if or not this is really the case - in situations where limits do not exist and neither weak limits nor sublimits are likely to represent, for some reason, a satisfactory alternative. So, here are my questions:

>> **Q1.** Is $\zeta \ast \bf C$, up to equivalence, a disguised form of anything familiar to you? **Q2.** Is it maybe a particular colimit (see note 2)? **Q3.** Does it satisfy any "obvious" universal property (see note 2)?

Thanks in advance, as always, for any hint.

**Remarkably useless notes.** (1) Ordinals have nothing special here, but since I'm working in TG, there is no loss of generality in using ordinals as indexing sets, of course. (2) Say, as an object of ${\bf Cat}(\mathcal U)$, for a sufficiently large universe $\mathcal U$.