The galaxy presents a disk-like morphology, though with noticeable disturbances. A faint, diffuse halo surrounds a more concentrated central region. There is evidence of possible ongoing or recent merger activity, indicated by asymmetries and irregularities in the disk structure. The disk appears relatively blue, suggesting active star formation. There are some indications of disturbances or tidal features, possibly resulting from the merger. Overall, the galaxy does not appear to be a classical spiral or elliptical, and exhibits characteristics of a galaxy undergoing some form of interaction or transformation.
