The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity towards the outer edges. There is little evidence of distinct spiral arms or a prominent disk. The color is primarily a yellowish-white, suggesting a stellar population dominated by older stars. There may be some subtle blue tinges in some regions. Based on its color and smooth structure, this galaxy is likely a mature system with relatively low ongoing star formation. There is no visual evidence of significant tidal features, major disturbances, or an active galactic nucleus.
