The galaxy presents as a relatively smooth, centralized luminous object. Its overall morphology appears elliptical to round. The color profile suggests a dominant older stellar population, with a general yellow-orange hue. There is a noticeable lack of distinct spiral arm structures or significant dust lanes; this further supports the likelihood of it being an elliptical galaxy. Signs of recent or ongoing star formation are subtle, with no apparent bright blue regions indicative of young, hot stars. The galaxy's profile is centrally concentrated, with a gradual decrease in luminosity towards its outer edges. There is no obvious evidence of a major merger event or significant tidal disturbances, as the outer regions are relatively smooth and symmetrical.
