The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. There is an elliptical appearance to the main body of the galaxy, with a slight elongation along one axis. The central region displays a bright, concentrated luminosity, suggesting a significant stellar population and/or active galactic nucleus. The color profile indicates a general yellowish-white hue, likely representing a mix of stellar populations. Subtle hints of bluer regions are visible around the central portion, potentially indicative of ongoing star formation. There is no strong evidence of spiral arm structures or significant dust lanes, although it is difficult to tell due to resolution. Overall, the galaxy appears to be relatively undisturbed, with no obvious signs of major mergers or tidal interactions. A more rounded, regular form is evident. It does not appear to be undergoing a major merging event, although minor disturbances cannot be ruled out.
