The galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse morphology. There is a centrally concentrated bulge of old stars, indicated by a yellowish-white hue. The overall shape is relatively round, with a slight elongation. There's a subtle hint of tidal disturbance or possible merging activity, but it is not definitively a merger. The light profile is smooth, with no apparent spiral arms or distinct dust lanes visible. There is a potential for a slight tidal tail to the south. Overall it appears to be a relatively old galaxy with weak current star formation.
