The galaxy presents as a largely smooth, elliptical-like structure. It appears to be slightly elongated, with a cigar-shaped morphology, though predominantly in-between round and elongated. A bright, concentrated central bulge is visible, suggesting a significant concentration of stars and possibly a supermassive black hole. The light distribution decreases gradually from the core towards the edges, displaying a diffuse halo, which indicates an older stellar population. There seems to be a slight bluing in areas around the central bulge, hinting at some star forming regions. The structure of the galaxy appears to be relatively undisturbed, indicating that it has likely not undergone a major merging event recently, but the minor disturbance cannot be ruled out. The galaxy exhibits an overall blue-ish white hue, indicative of ongoing star formation and intermediate-age stellar populations mixed with evolved stars.
