The galaxy exhibits a disk-like morphology, seen at a significant inclination. The central region is bright and concentrated, potentially indicating the presence of a bulge. A ring-like structure surrounds the core, displaying variations in color, with tinges of blue and green suggesting active star formation in these regions. The outer disk appears fainter and more diffuse, with hints of a spiral arm structure extending from the central region. There is some evidence of disturbances in the outer disk, possibly from interactions. Overall, the galaxy shows characteristics consistent with a spiral or lenticular galaxy with ongoing star formation within a central ring.
