This galaxy presents as a likely interacting system, exhibiting morphological distortions indicative of gravitational interaction. There is a clear separation into two dominant components: one component appears relatively smooth and rounded, with a concentrated, bright core, displaying a blue-shifted spectral appearance. The other component exhibits a more elongated and amorphous structure, displaying a red-shifted spectral appearance and a less defined nucleus.

A faint bridge of material appears to connect the two components, suggesting tidal interactions. There are some disturbances apparent in the disk, possibly some signs of tidal tails, which are consistent with a merging event in progress. The overall morphology is not consistent with a relaxed elliptical or spiral system, pointing towards a dynamic, actively evolving structure.
