The galaxy presents an intermediate morphology, displaying characteristics of both elliptical and spiral galaxies. The central bulge is prominent and appears relatively smooth, contributing to a substantial fraction of the galaxy's overall light. There is evidence of a disk component, though it appears somewhat disturbed or irregular.

The overall shape exhibits a degree of roundness but leans towards being in-between round and elongated. It is currently undergoing some type of merger, showing signs of significant disturbance. There is noticeable asymmetry, and it looks like it's actively merging with another galaxy.

Based on the apparent colors, it seems to have ongoing star formation activity.
