The galaxy presents as a single, centrally concentrated object. It exhibits a primarily smooth morphology, with a roughly circular shape in the observed plane. The core region displays a notable yellowish-white hue, suggesting an older stellar population or a significant amount of dust obscuration. There's some evidence of a faint, diffuse halo or extended structure surrounding the central region. A slight asymmetry may be present, with a possible faint extension or tidal feature on one side, hinting at a past or ongoing interaction. Overall, the galaxy appears relatively undisturbed, consistent with a relaxed, late-type system, although some minor disturbances cannot be ruled out entirely. The integrated light from the galaxy indicates that the object is relatively luminous.
