The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology with little evidence of spiral arms or significant substructure. The overall color appears yellowish-white, suggesting a dominant population of older stars. The light is relatively uniform across the galaxy's body, which indicates that the bulk of the star formation is likely suppressed. The galaxy is elliptical in shape. There are is no visible ongoing major merger or significant tidal disturbance that is detected.
