The galaxy presents a generally elliptical morphology, exhibiting a smooth, centrally concentrated luminosity profile with a high degree of overall symmetry. The core region is characterized by a yellowish-orange hue, potentially indicative of an older stellar population. There is some indication of a faint, bluer extension or possible tidal feature projecting outwards. This could be a very faint arm, or perhaps an artifact. There are no signs of prominent spiral arms or a well-defined disk structure. It appears to be an early-type galaxy undergoing minimal current star formation. A mass estimate suggests it is likely a very massive galaxy. The high roundness factor suggests this object is nearly circular and not elongated. It may be undergoing or have recently undergone minor interactions with a companion galaxy, indicated by the faint protrusion.
