The galaxy presents as a lenticular or early-type spiral, characterized by a smooth, diffuse central bulge that transitions into a fainter, elongated disk. There is an overall cigar-like shape. The central region exhibits a yellowish hue, potentially indicative of an older stellar population. The outer regions of the disk appear bluer. The structure appears largely undisturbed, with no obvious signs of tidal features, prominent dust lanes, or ongoing major mergers. Star formation activity appears low.
