The galaxy presents as an elliptical or lenticular type, exhibiting a primarily smooth morphology with a concentrated central bulge. The overall shape appears relatively round. There's some subtle indication of a disk-like structure, but the light is dominated by the bulge component. The color distribution indicates that the stellar population consists mainly of older stars, with a redder hue dominant throughout the galaxy except for the central portion which appears bluer. There may be a low level of ongoing star formation, but it is not contributing significantly to the overall color. A faint, extended halo may be present, gradually fading into the background sky. There's also some evidence of a minor tidal disturbance or interaction occurring, as one side of the galaxy seems slightly extended or disrupted. No prominent dust lanes or spiral arms are visible.
