The galaxy presents an overall smooth morphology, with a concentrated central bulge. The galaxy appears to be elliptical, with a slight elongation along one axis. The core region exhibits a reddish hue, potentially indicating an older stellar population. The outer regions of the galaxy gradually fade into a bluer color profile, which may suggest ongoing star formation or a younger population of stars. There is no strong evidence of spiral arm structures, or significant dust lanes. Overall, the galaxy appears to be relatively undisturbed with no apparent signs of recent major mergers or tidal interactions.
