The galaxy presents a largely smooth, elliptical morphology. The light is centrally concentrated, with a gradual decrease in luminosity as one moves outward from the core. The galaxy appears quite round in shape. There is no evidence of spiral arms or a prominent disk structure in this image. There are no obvious signs of recent or ongoing major merger activity or significant tidal disturbances. The galaxy's color appears yellowish, suggesting a population dominated by older stars, consistent with a relatively low ongoing star formation rate.
