The galaxy presents as a single, relatively smooth, elliptical structure. There is a bright central bulge with a gradual decrease in luminosity towards the outer edges. The colour gradient suggests a population of older stars, contributing to the overall yellowish hue, particularly concentrated towards the center. No distinct spiral arms or features indicating active star formation are readily apparent, though some subtle colour variation is visible in the outer regions. The shape is elongated, but without strong signs of tidal disturbances or a major ongoing merger event, although a minor interaction cannot be ruled out.
