The galaxy presents as a largely featureless, smooth elliptical. It exhibits a concentrated, bright central bulge that gradually fades into the outer regions. There is no apparent disk structure, spiral arms, or significant dust lanes. The overall color is yellowish-red, suggesting an older stellar population and relatively low ongoing star formation. The galaxy's morphology appears undisturbed, without signs of recent or ongoing major merger events. It is approximately circular. The color gradient indicates potential metallicity variations, with a possibility of more metal-rich stars concentrated toward the center. The observed characteristics point to a galaxy that has likely undergone significant evolution, with star formation processes gradually declining over time.
