The galaxy presents as a luminous, centrally concentrated object. It exhibits a largely smooth morphology, with a dominant elliptical profile. There is a subtle suggestion of spiral arm structure or a faint disk-like component, but this is not clearly defined. A slight asymmetry in the light distribution, with a small plume or tidal feature extending from the galaxy, hints at possible gravitational interactions or a minor merger event in its past. The color is generally consistent with an older stellar population, but there is a small amount of light suggesting active star formation. There is an object nearby that appears to have a tidal feature as well, which may mean that the tidal plume is due to the two galaxies interacting.