The galaxy presents as a luminous, somewhat rounded structure. A concentrated central bulge dominates the overall morphology, displaying a smooth, yellowish-white hue indicative of an older stellar population. Fainter, diffuse extensions surround the core, exhibiting a slightly bluer tint that suggests the presence of more recent star formation. These outer regions appear relatively unstructured, lacking prominent spiral arms or well-defined features. There is a subtle hint of asymmetry in the overall shape, potentially indicative of past interactions or mergers.
