The galaxy presents as a relatively smooth, cigar-shaped structure with a dominant central bulge. The luminosity appears concentrated towards the center, suggesting a higher density of older stellar populations in that region. The outer regions exhibit a gradual decrease in surface brightness. There's a hint of faint, disk-like structure. The overall color is consistent with an evolved stellar population, with a slight bluer tinge, possibly indicating recent though suppressed, star formation activity. There are no obvious signs of major mergers or significant tidal disturbances, although minor asymmetries are present. The object appears to be relatively isolated, without close companion galaxies.
