The galaxy appears as a luminous, centrally concentrated object. It exhibits a largely smooth morphology, though some subtle features suggest a possible disk-like structure. The central region is bright, with a yellowish hue. This likely indicates an older stellar population. The outer regions show a gradual decrease in brightness and a bluer color, suggesting ongoing, though limited, star formation. There is no strong evidence of a recent major merger event, and the galaxy appears relatively undisturbed. Faint spiral arms may be present, but are not clearly defined due to the smoothing effect of the image. The overall shape appears largely elliptical, with a moderate degree of roundness.
