The galaxy presents as a relatively compact object with a smooth, diffuse light profile. It exhibits a generally elliptical morphology, appearing mostly rounded in shape with no strong evidence of spiral arm structure. There is a suggestion of a slight elongation, but overall, the galaxy's light is concentrated in a centrally dominant, seemingly undisturbed spheroid. The color appears to be a yellowish-white, which may indicate an older stellar population. There are no apparent tidal tails or other signs of major ongoing mergers, although a slight irregularity in the light distribution suggests possible minor disturbances or interactions.
