This galaxy exhibits a primarily smooth morphology, with a slight elongation in its overall shape. The central region displays a higher concentration of light, appearing as a diffuse, brighter core. The color profile suggests an older stellar population dominating the galaxy's composition, particularly within the central bulge, which appears more reddish. There is some evidence of bluer regions, possibly indicating areas of recent or ongoing star formation, primarily located away from the central bulge. A possible tidal feature is present, indicating a past interaction. There is little indication of well-defined spiral arm structure or a prominent dust lane within the visible spectrum. The lack of strong features and smoothness of the light distribution are consistent with an elliptical or lenticular galaxy classification.
