The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. Its overall shape appears nearly circular, with no obvious distortions or tidal features indicative of recent major merger activity. There is a concentration of light toward the galaxy's center, implying a significant bulge component. The color profile is relatively uniform, displaying a general blue-white hue, but the central region is a very bright white color. No distinct spiral arms or prominent dust lanes are apparent in this image. The galaxy has a very smooth texture. Given the smooth appearance, round shape and uniform color profile, this galaxy may be an elliptical galaxy that has undergone past mergers, but is not currently involved in any merger activity. Star formation is likely present but low, consistent with a more evolved stellar population. The galaxy exhibits a faint but non-negligible disk component.
