The galaxy presents as a relatively smooth, elliptical structure. It exhibits a moderate degree of elongation, appearing more 'in-between' round and cigar-shaped. The central region displays a concentration of light, suggesting a bulge. Faint disturbances are visible around the galaxy, possibly indicative of minor interactions. There appears to be a slight color gradient, with bluer hues concentrated towards one end, suggestive of some star formation activity, and redder hues dominating the other. The overall structure does not appear to be heavily disturbed or actively merging, though some asymmetries hint at past or ongoing interactions.
