The galaxy appears as a largely featureless, elliptical-shaped structure with a smooth light distribution. It exhibits a concentrated central bulge that gradually fades into its outer regions. There is little evidence of spiral arms or significant dust lanes. The galaxy displays a predominantly yellowish-red hue, which suggests an older stellar population and reduced current star formation. There are no indications of active galactic nuclei (AGN) activity or any significant tidal disturbances, suggesting it is an isolated galaxy that has not recently undergone a major merger. Overall, the galaxy presents characteristics of a quiescent, relatively evolved system.
