This galaxy presents as a mostly featureless, smooth object with an elliptical morphology. The light distribution appears centrally concentrated, with a gradual decrease in surface brightness outwards from the core. The core region exhibits a yellowish-white hue, potentially indicating an older stellar population. The outer regions are significantly fainter, displaying a very subtle blue shift, which might indicate some more recent star formation, though it is difficult to assess with certainty. There is no evidence of spiral arms, bars, or significant dust lanes. No obvious tidal features or signs of ongoing mergers are observed, though very minor disturbances cannot be ruled out at this resolution. Overall, the galaxy appears to be a relatively evolved system.
