The galaxy presents as a slightly elongated, disk-shaped structure with a bright central bulge. The overall color suggests a mixture of stellar populations, with a central concentration of older stars and possibly some ongoing star formation in the outer regions. The ellipticity is noticeable but not extreme. There is a slight asymmetry in the disk, hinting at possible tidal interactions or recent minor mergers. A faint, extended halo may be present, though difficult to discern definitively.
