The galaxy presents as an elliptical morphology, exhibiting a smooth, centralized luminosity profile. There is an apparent lack of distinct spiral arm structure. The central bulge appears prominent and bright, with a gradual decrease in luminosity towards the outer regions. The overall shape is mostly rounded, though there is a slight elongation giving it a somewhat lenticular appearance. There may be the possibility of faint disturbance or tidal features extending from the main body of the galaxy, though the resolution makes this difficult to determine definitively. The galaxy’s color profile suggests a population of older stars, lending to the smoother appearance and lack of intense star formation regions. There is no indication of a major merger in progress, and while minor disturbances are possible, the overall structure indicates a relatively relaxed, evolved system.
