The galaxy presents as a lenticular or early-type spiral, observed at a significant inclination to our line of sight. The central bulge appears prominent and exhibits a yellowish hue, suggesting a population of older stars. A faint, bluish disk surrounds the bulge, indicating the presence of some younger stellar populations and potential ongoing star formation. The disk appears relatively smooth, lacking distinct spiral arm structures. The overall shape of the galaxy is elongated, with the major axis significantly longer than the minor axis. The surface brightness distribution appears to be centrally concentrated, with a gradual decrease in intensity outward from the bulge. There is a faint, diffuse halo surrounding the main body of the galaxy.
