The galaxy presents as a single, cohesive structure with a smooth, centrally concentrated light profile, typical of an elliptical morphology. It exhibits a moderate degree of ellipticity, appearing somewhat elongated with a cigar shape. The central region of the galaxy is characterized by a yellowish-orange hue, suggesting an older stellar population with a relatively low rate of recent star formation. This contrasts with the fainter, bluer outer regions, which may indicate the presence of younger stars or ongoing, but limited, star formation activity. There are no discernible tidal features or significant morphological disturbances, implying that it is a relatively undisturbed system, and most likely not undergoing major mergers.
