The galaxy exhibits a generally smooth morphology, lacking discernible spiral arms or a prominent disk structure. It is characterized by a centrally concentrated bulge with a gradual decrease in luminosity towards its outer regions. The light distribution appears relatively symmetric and elliptical. There is a subtle color gradient, with the central region appearing more yellow, potentially indicating an older stellar population or a higher concentration of dust. The galaxy displays minimal evidence of ongoing mergers or tidal disturbances in its immediate vicinity.
