The galaxy presents a somewhat elliptical morphology. The central bulge appears bright and concentrated, exhibiting a yellowish-white hue suggestive of an older stellar population. A fainter, more diffuse disk surrounds the bulge, with a subtle greenish tint. The disk appears relatively smooth, lacking prominent spiral arm structures or significant dust lanes. There is no obvious presence of a bar structure. The overall appearance suggests a galaxy undergoing a relatively low rate of star formation. The galaxy appears to be relatively isolated, lacking obvious signs of ongoing or recent major mergers.
