The galaxy presents as a relatively smooth, centrally concentrated structure. Its morphology is suggestive of an elliptical or lenticular type. The central region exhibits a bright, slightly yellowish hue, which may indicate an older stellar population. Moving outward from the center, the light diffuses into a fainter, bluer halo, possibly indicating a small amount of star formation is happening. The shape of the galaxy is approximately round, with only a slight deviation toward an elongated form. There appear to be some disturbances, indicating a past merger or tidal interaction, but they do not appear to be ongoing at this time. Overall, the galaxy appears to be a mature system with modest recent activity.
