The galaxy appears as a centrally concentrated, relatively smooth object. Its overall shape is ellipsoidal, tending toward round rather than highly elongated. A bright core region dominates the central part of the galaxy. A diffuse halo surrounds the core, fading gradually outwards. The color profile suggests a redder hue in the outer regions compared to the central core, which exhibits bluer tones. There is no clear evidence of spiral arms or distinct features indicating ongoing major mergers or significant tidal disturbances, although there is a slight asymmetry visible that may indicate a past minor interaction. Star formation is likely occurring at a low rate, primarily concentrated in the central regions as evidenced by the blue hue.
