The galaxy presents as a lenticular or early-type spiral galaxy, characterized by a dominant, smooth bulge and a faint, flattened disk. The central region exhibits a high concentration of light, suggesting an older stellar population. There is minimal evidence of spiral arm structure or active star formation within the disk, which appears relatively uniform in color and luminosity. The overall morphology indicates a system that is likely undergoing, or has already completed, a transition from a more actively star-forming spiral to a quiescent, bulge-dominated system. The shape deviates from being perfectly round, leaning towards being cigar shaped indicating some degree of inclination from our vantage point. There are no obvious signs of major tidal disturbances or ongoing mergers.
