This galaxy appears to be a spiral galaxy, seen at an oblique angle. It possesses a noticeable central bulge that appears relatively small compared to the overall disk. The spiral arms are clearly visible, and appear to be grand design, extending outwards from the central bulge. The winding of the spiral arms appears to be of medium tightness. Star formation is evidently active, as indicated by the blue color, particularly prominent within the spiral arms, suggesting the presence of young, hot stars. There is no obvious dust lane visible. There are hints of a potential weak bar structure in the central region. Based on the disturbed morphology it is likely undergoing some level of interaction with another galaxy. There is no apparent evidence of a major merger however.
