The galaxy presents as a relatively smooth, elliptical-shaped structure with a bright, concentrated central bulge. There appears to be a significant decrease in luminosity extending outward from the core, with faint, diffuse edges. The galaxy exhibits a slightly elongated morphology. The overall color profile suggests a population of older stars, with a subtle reddish hue throughout the galaxy. No distinct spiral arms or prominent dust lanes are visible. There is no indication of ongoing major merger activity or significant tidal disturbances, suggesting a relatively undisturbed and evolved system.
