The galaxy presents as a primarily smooth, elliptical-like structure, characterized by a concentration of light towards its center. There is a discernible, yet subtle, decrease in luminosity extending outwards from the core. The galaxy exhibits a generally rounded morphology, with a slight deviation towards an elongated shape. No obvious spiral arms or significant dust lanes are detected. Overall the galaxy looks isolated, showing no strong indications of recent or ongoing major merger activity or significant tidal disturbances. The galaxy appears to be relatively evolved, consistent with a population dominated by older stars, giving it a reddish hue.
