The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a notable central bulge. The light distribution suggests a high concentration of stars in the core region, gradually decreasing towards the outer edges. The overall color is yellowish, which implies an older stellar population with fewer hot, young stars and a greater abundance of red giants. The shape appears slightly elongated rather than perfectly spherical, with a suggestion of a disk. There is no apparent active star formation, though the blueish colour in the top-left suggests potential activity. It does not appear to be undergoing a major merger, though it could be interacting with smaller bodies.
