The object appears to be a spiral galaxy, observed face-on or at a slight inclination. It exhibits well-defined spiral arms that are tightly wound around a central bulge. The bulge appears relatively small in comparison to the disk, presenting as a somewhat diminished central concentration of light. The spiral arms show evidence of active star formation, indicated by regions of bluish light, likely corresponding to populations of young, hot stars. Some arms are difficult to distinguish due to lack of clarity or low intensity. There is no apparent evidence of a major merger or significant tidal disturbance affecting the overall structure of the galaxy. A faint bar structure is possibly present within the central region, with an orientation that is oblique relative to the major axis of the disk. The galaxy is possibly undergoing a low level of star formation.
