The galaxy presents as a lenticular or possibly an elliptical galaxy. It exhibits a generally smooth light distribution, with a highly concentrated central bulge. The overall shape is elongated, with an apparent ellipticity. The color gradient shows a redder core transitioning to slightly bluer outer regions, suggestive of an aging stellar population in the central regions and possibly some ongoing, but low, star formation in the outskirts. There is no distinct dust lane or prominent spiral arm structure visible in this image. The galaxy appears relatively isolated and does not exhibit any obvious signs of interaction or recent merger events.
