The galaxy appears as a single, mostly homogenous object with a smooth and rounded morphology. The color profile shifts gradually from a somewhat reddish central region to a slightly greener surrounding area. No distinct spiral arms or bar structures are visible. There are no obvious signs of recent major mergers or significant tidal disturbances. The light profile is quite concentrated, indicating that the majority of the galaxy's light is emitted from the core. The observed properties suggest that the galaxy is likely an elliptical galaxy.
