The galaxy presents as a largely featureless, elliptical-like structure. Its overall color appears to be a somewhat red, indicative of an older stellar population. The galaxy displays a high degree of central concentration, with a bright core that fades outward into a more diffuse halo. There is little indication of spiral arms or significant dust lanes. The overall shape is close to round, showing only slight ellipticity. There is no strong evidence of ongoing major merging activity, though the potential for minor disturbances or past merger events cannot be completely ruled out based on the image alone.
