The galaxy presents as a lenticular, cigar-shaped structure, elongated along its major axis. A prominent central bulge is observed, contributing significantly to the galaxy's overall luminosity. The disk component appears relatively smooth, lacking significant spiral arm structure or prominent dust lanes. The galaxy exhibits a color gradient, with the central bulge displaying a slightly yellower hue compared to the disk, possibly indicating an older stellar population concentrated in the bulge. There is a subtle suggestion of tidal disturbances, although these features are not overtly pronounced. No clear signs of active galactic nuclei activity, such as bright emission lines, are immediately apparent.
