The galaxy presents an elliptical morphology, exhibiting a smooth light distribution with a high degree of central concentration. There is no apparent structure such as spiral arms or a distinct bar. The galaxy displays a gradient in color, with the core appearing more yellow/white and the outer regions slightly bluer, suggesting some level of on-going star formation or a younger stellar population in the outskirts, though the galaxy is likely dominated by older stars. There is no obvious dust lane obscuring the galaxy's features, nor any indications of significant tidal distortions or ongoing mergers. The light profile appears relatively undisturbed, indicating a dynamically relaxed system.
