The galaxy presents as a concentrated, centrally-dominated system. Its morphology appears relatively smooth and elliptical, with a notable lack of distinct spiral arm structures. The light profile suggests a centrally concentrated bulge, transitioning smoothly outwards to a fainter halo. Color gradients indicate a redder core, potentially indicative of an older stellar population. The overall shape is somewhere between round and elliptical, though closer to being round. There is no strong evidence of a major merger, although subtle distortions or minor disturbances may be present in the outer regions. Overall the galaxy appears to be relatively massive.
