The object appears to be a spiral galaxy, oriented approximately face-on. It exhibits a distinct central bulge with a moderate size relative to the galactic disk. Two prominent spiral arms emanate from the central region and wind around it. The arms present a fairly tight winding pattern. The arms show evidence of active star formation regions, as indicated by their bluer hue, which could indicate the presence of younger, hotter stars. The disk component is the dominant structural feature. There is no obvious, strong bar-like structure apparent in the central region. The overall morphology suggests that this galaxy is likely not undergoing a major merger, although there might be subtle disturbances. The galaxy displays intermediate luminosity, with its blue color revealing information regarding its stellar populations and possible star formation.
