The galaxy presents as an elliptical, disk-like structure, visibly inclined relative to the observer. The central bulge appears prominent and concentrated, with a smooth, yellowish color suggesting an older stellar population. Diffuse arms extend from the bulge, displaying a bluer color. A smaller, distinct component appears separated, yet connected, perhaps the result of a recent or ongoing interaction. The object exhibits a low degree of rotational symmetry. The galaxy overall has a low surface brightness.