This galaxy presents as a relatively smooth, centrally concentrated object. The light profile suggests a dominant bulge component, with a gradual decline in surface brightness moving outward from the core. There is a subtle color gradient noticeable within the galaxy. The central region exhibits a warmer hue, trending towards redder wavelengths. The surrounding disc/halo appears bluer.

While the overall morphology seems undisturbed, there may be a faint tidal feature or asymmetry on one side, which could be indicative of minor past interaction. Further analysis is needed to confirm this observation, as it could also be due to a subtle imaging artifact.

The integrated color of the galaxy indicates the presence of an evolved stellar population, however some star formation cannot be ruled out due to the bluer outer regions.
