The galaxy presents as a relatively smooth, elliptical-like structure. Its light is concentrated towards the center, appearing as a bright, somewhat diffuse core. The overall shape is elongated, deviating moderately from a perfect circle. There are no prominent spiral arms or distinct disk-like features readily visible. There is some indication of minor asymmetry or a faint tidal feature on one side, suggesting the possibility of a past interaction or minor disturbance. The color profile indicates a population of older stars. The galaxy appears to have a moderate mass and a comparatively low rate of star formation.
