The galaxy appears to be a relatively smooth, elliptical galaxy exhibiting a somewhat spherical shape. Its core presents a bright, concentrated luminosity that gradually decreases towards the outer edges of the galaxy. The color profile suggests a population of older stars, resulting in a reddish-yellow hue concentrated towards the center. There is no readily apparent spiral structure, bar, or significant dust lane obscuration. It shows no obvious signs of major ongoing merging activity or tidal disturbances. Its smooth morphology suggests it may be a relatively quiescent system.
