The galaxy presents a primarily smooth, elliptical morphology. It appears moderately rounded, with a slight elongation suggesting a shape between circular and cigar-like. There's a subtle hint of a disk-like structure, but the overall light distribution is dominated by a bulge. The central region shows a concentration of light, appearing yellowish-orange, which might indicate an older stellar population. The outer regions fade gradually, exhibiting a bluish-white hue possibly suggesting the presence of some younger stars, or low-level star formation. There seems to be no indication of ongoing major merger activity. The overall structure appears relatively undisturbed, and there might be minor disturbances.
