The galaxy presents as a slightly inclined spiral, approximately 3.5 arcseconds in radius. It exhibits a prominent, bright central bulge with a yellow hue, suggesting an older stellar population. The surrounding disk displays a bluer color profile, hinting at ongoing star formation, albeit at a relatively low rate. There is some indication of spiral arm structure, though these features are not sharply defined, appearing somewhat diffuse. The overall shape is more elliptical than circular. There is no obvious evidence of a major ongoing merger. A subtle asymmetry in the disk suggests the possibility of minor tidal interactions or past disturbances.
