This galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentration of light, indicative of a bulge, which fades gradually outwards. There is little evidence of distinct spiral arms or features typically associated with disk galaxies. The overall color is primarily pale, with subtle variations, suggesting a mix of stellar populations. It exhibits little morphological disturbance, with no clear signs of on-going or recent major merger activity. Some subtle asymmetry may be present in the outer regions.
