The galaxy presents as a relatively smooth, elliptical-like structure. The core region displays a pronounced concentration of light, appearing brighter and more reddish in color compared to the surrounding areas. The outer regions exhibit a gradual decrease in luminosity, with a more greenish hue. There is no readily apparent spiral structure or significant dust lane features. The overall morphology suggests a well-mixed stellar population, likely dominated by older stars. There is no obvious evidence of recent or ongoing major merger activity or significant tidal disturbances. The galaxy is appears mostly rounded in shape.
