The galaxy presents a generally elliptical morphology. It exhibits a smooth appearance, with no distinct spiral arms or bar structure readily discernible. The central bulge is prominent, displaying a concentrated, bright core. A gradual decrease in luminosity extends outwards from the core. The color profile suggests a population of older stars, with a relatively redder hue overall. There are no apparent signs of ongoing major mergers or significant tidal disturbances, though some minor asymmetry is observed.
