The galaxy presents as a primarily smooth, elliptical-like structure with a concentrated, bright central region, suggestive of a significant bulge component. There is a subtle color gradient, with the core appearing slightly yellower, likely indicating an older stellar population and/or significant dust obscuration there. The outer regions exhibit a bluer hue, which might indicate the presence of younger, hotter stars and ongoing star formation. The galaxy exhibits a minor degree of asymmetry and potentially some faint, subtle features hinting at a past or ongoing minor interaction or disturbance, although these are not prominent. The shape is generally in between being perfectly round and cigar-shaped.
