The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a roughly circular or elliptical shape, though there are some subtle asymmetries in its outer regions. The light distribution shows a central bulge that transitions into a broader disk-like component. Faint, diffuse features can be seen extending from the main body of the galaxy, suggesting tidal interactions or recent minor merger activity.

The color gradients within the galaxy show a distinct pattern. The central region is dominated by yellowish-white hues, indicative of an older stellar population. The outer disk regions display a bluer tint, which might indicate regions of ongoing star formation. The presence of these differing color populations suggests an evolutionary history that includes both quiescent and active star-forming phases. The overall shape and color distribution lead to a classification as an intermediate-type galaxy, possibly a late-type spiral or an early-type elliptical.
