The object presents as a diffuse, centrally concentrated, and seemingly compact galaxy. It exhibits a moderate degree of smoothness, with a fraction of the overall light distribution appearing somewhat unstructured. There is no distinct disk structure readily apparent, and the light profile suggests a generally elliptical morphology. 

Evidence for tidal disturbances or ongoing mergers is marginal. No extended tidal tails or bridges are immediately obvious. The majority of the galaxy's light is concentrated within a small region, with colors ranging from redder hues in the core to slightly bluer tints in the outer regions. The galaxy has no central bulge that is brighter than the rest of the galaxy. The data are consistent with a faint elliptical galaxy, potentially with a small degree of interaction history.
