The object presents as a relatively smooth galaxy, approximately elliptical in shape. It displays a concentrated central bulge that is somewhat diffuse. The color gradient suggests a population of older stars, evidenced by the reddish-yellow hue towards the central region and the more moderate intensity blue light present towards the outer halo, though this could also be dust within the disk. No distinct spiral arms are visible. There's little evidence of significant star formation activity or major disturbances in its structure, although there are faint irregular extensions that could indicate ongoing tidal interactions or minor mergers. The galaxy appears to be a relatively evolved system.
