The galaxy presents as an elliptical morphology, displaying a smooth, centrally concentrated light distribution. The core region exhibits a yellowish-orange hue, potentially indicative of an older stellar population. Moving outward from the core, the color gradually transitions to a bluer, more diffuse halo. No distinct spiral arms or bar structures are discernible. There appears to be no ongoing major merger event, although the morphology is slightly disturbed. The galaxy appears relatively isolated, without any obvious signs of tidal interactions with nearby galaxies. The light profile suggests a relatively evolved system with a moderate amount of star formation activity.
