The galaxy presents as a centrally concentrated object with a predominantly smooth morphology. The light distribution suggests an elliptical form, tending toward roundness, although not perfectly spherical. There is a subtle color gradient, with the central region exhibiting a yellowish-white hue, possibly indicating an older stellar population, and the outer regions showing a very faint bluish tint, suggesting some ongoing, albeit subdued, star formation. There is no evidence of prominent spiral arms or other significant disk structures. The galaxy appears relatively undisturbed, with no signs of ongoing major mergers or significant tidal disruptions. A very subtle asymmetry may be present on one side, suggestive of a minor interaction or internal dynamic process. The galaxy exhibits moderate luminosity, indicating an intermediate absolute magnitude.
