The galaxy appears as a somewhat elongated, elliptical-like structure. It displays a relatively smooth overall morphology, with no prominent spiral arms or bar features immediately discernible. A bright central bulge is present, suggesting a concentration of older stars toward the core. The galaxy exhibits a gradual decrease in surface brightness moving outward from the center, with a somewhat diffuse outer halo. Faint, blue-ish light is detected in the outer regions. The galaxy's shape is in between round and cigar-shaped, it is not perfectly circular. There is no obvious evidence of major mergers or significant tidal disturbances impacting the galaxy's overall structure; the galaxy shows no signs of interactions with nearby galaxies.
