The galaxy presents as a centrally concentrated object with a generally smooth appearance. Its shape is approximately elliptical, displaying a moderate degree of ellipticity without being overly elongated. A bright central region dominates the structure, suggesting the presence of a concentrated core, possibly harboring a supermassive black hole. The color gradient transitions from a bluer central region to redder outer regions. No distinct spiral arm structures or prominent dust lanes are visible. There are no obvious signs of recent or ongoing major mergers, though minor disturbances may be present. Overall, the galaxy appears to be a relatively evolved system, likely an early-type galaxy with a stable morphology.
