The galaxy appears as a centrally concentrated, elliptical or lenticular type. Its overall color suggests a relatively older stellar population, with a yellowish-orange hue dominating. There is a smooth distribution of light, with no apparent spiral arm structures or significant dust lanes visible. The central bulge is prominent, showing a gradual decrease in brightness toward the outer regions. There is little evidence of recent or ongoing star formation, based on the lack of blue light. No signs of tidal disturbances, mergers, or active galactic nuclei activity are apparent in the image. The galaxy displays a generally round appearance.
