The galaxy appears as a centrally concentrated object with a smooth light distribution, indicative of an elliptical morphology. The core exhibits a bright, relatively compact structure. Moving outward from the center, the intensity of the light decreases smoothly, with no discernible spiral arm structure. The overall color appears somewhat redder, suggesting a population dominated by older stars and a comparatively low rate of on-going star formation. There is no obvious evidence of significant dust lanes or tidal features, indicating a relatively undisturbed system, with low chances of ongoing merging events or major disturbances. The galaxy's shape is close to round.
