The galaxy presents a generally smooth morphology, exhibiting a centrally concentrated, bright core that gradually fades into a diffuse halo. The color profile suggests a population of older stars, with a yellowish hue dominating the central region. There is little evidence of spiral arms or significant dust lanes within this galaxy. The overall roundness suggests a classification leaning towards elliptical. Faint, asymmetric extensions may indicate tidal interactions or minor disturbances. Overall the galaxy appears quite massive.
