The galaxy appears to be a spiral galaxy, potentially undergoing a merger. It displays a relatively diffuse structure, lacking a well-defined, centralized bulge. There is evidence of tidal features or distortions in the disk, particularly on the upper side of the galaxy, suggesting gravitational interaction with another galaxy. The disk itself seems to be moderately inclined with respect to our line of sight. There appears to be a relatively high amount of recent star formation, given its absolute magnitudes, as indicated by the presence of clumpy, blue regions within the disk. These regions may represent active star-forming regions. The galaxy appears to be of intermediate mass, neither a dwarf nor a giant galaxy. It also displays a small bulge fraction and a significant disk component.
