The galaxy presents as an elliptical morphology. It exhibits a generally smooth light distribution, with a centrally concentrated bulge that fades towards the outer regions. The color gradient suggests the core is comprised of older stars that are more yellow, while the outer regions appear slightly bluer, indicating a population of younger stars. There's a slight elongation to the galaxy's shape, appearing more cigar-shaped than perfectly round, but it lacks any distinct features such as spiral arms or a prominent disk. There's no evidence of significant ongoing mergers or major disturbances in its morphology.
