The galaxy appears as an elliptical or lenticular structure, exhibiting a generally smooth and featureless morphology. It displays a centrally concentrated luminosity profile, with a gradual decrease in brightness towards its outer regions. Its shape is moderately elongated. There are no indications of prominent spiral arms or a well-defined disk. The galaxy's color index suggests the presence of an older stellar population, with a redder appearance in the central bulge and a slightly bluer hue in the outer regions, perhaps indicative of ongoing, low-level star formation. There's no visible evidence of major mergers or significant tidal disturbances.
