The galaxy presents as a relatively compact, lenticular-like object with an overall smooth appearance. The light is concentrated toward the center, with a gradual decrease in intensity towards the outer regions. There is very little evidence of spiral arm structures or prominent dust lanes.

The color profile suggests a population of older stars. The galaxy exhibits a slight elongation, but it appears primarily rounded. There is no obvious presence of a significant bulge or disk, suggesting a transitional morphology between elliptical and spiral forms. It also doesn't appear to be undergoing major mergers or gravitational disturbances, though there may be a hint of minor disturbance in the outer regions.
