The galaxy presents as a centrally concentrated, smooth object. The morphology suggests an elliptical or lenticular classification, evidenced by the lack of distinct spiral arms or prominent disk features. The light profile indicates a gradual decrease in luminosity from the core outwards, with no apparent substructure within the visible extent. The color is generally yellowish to reddish, suggestive of an older stellar population and reduced recent star formation activity. The galaxy appears relatively isolated, showing no signs of tidal interactions or ongoing mergers with other galaxies. Based on its estimated distance and apparent size, the galaxy is a relatively compact system.
