The galaxy presents as a relatively smooth, elliptical-like structure. The core region is distinctly brighter and exhibits a yellowish hue, suggestive of an older stellar population. A less luminous, somewhat bluer component is observed offset from the center, possibly indicative of a region with ongoing star formation activity or the remnant of a minor merger event. Faint, diffuse light extends from the central region, though its overall structure is difficult to discern with precision. The morphology implies that this galaxy could potentially be undergoing or have undergone a merging event.
