The galaxy presents a somewhat elongated morphology, appearing more cigar-shaped than round. The light distribution is not uniform; it seems to exhibit some substructure or features rather than being entirely smooth. There is no strong indication of a major ongoing merger event; however, there is a minor disruption or interaction evidenced within the galaxy's structure. The galaxy is likely a disk galaxy, as some disk features are present within its structure. The galaxy appears to be actively forming stars, with some regions showing signs of more intense star formation than others.
