The galaxy presents as a relatively smooth, elliptical-like structure, although there is some indication of a disk component. It appears moderately compact, with a concentrated central bulge that is bright. The overall color is yellowish, suggestive of an older stellar population. There's a slight asymmetry to the galaxy's shape, which may be indicative of a past or ongoing minor interaction or disturbance. There is no strong visual evidence of significant star formation, active galactic nucleus activity, or major mergers.
