The galaxy presents a largely smooth and elliptical morphology, with no discernible spiral arm structures or significant dust lanes visible. The light distribution is concentrated toward the center, exhibiting a bright, relatively compact core. The galaxy appears nearly round in shape, with a slight elongation. The color profile suggests a population of older stars. The outer regions show a gradual decrease in luminosity, transitioning into the background sky. There is no evidence of ongoing major mergers or tidal disturbances.
