The galaxy presents as a primarily smooth, disk-like structure with a prominent central bulge. The galaxy exhibits a relatively high degree of symmetry. The central bulge appears to be a dominant feature, with a concentration of light indicating a significant population of older stars or potentially an active galactic nucleus. Fainter, disk-like structures can be observed extending outwards from the central bulge. These extensions are characterized by subtle color gradients, suggesting the presence of ongoing or recent star formation. There is a possibility of minor disturbances in the overall structure, perhaps indicating a past or ongoing interaction with a smaller galaxy or gravitational perturbation. The overall form suggests a galaxy undergoing a transition from a spiral to an elliptical morphology, or perhaps a lenticular galaxy viewed close to edge-on.
