The galaxy presents a distinct spiral morphology. The spiral arms are tightly wound around a prominent central bulge. The bulge appears to be moderate in size relative to the overall disk. The arms display a somewhat flocculent structure, exhibiting some star formation. The colour gradient suggests active star formation within the arms, although the overall colour indicates that the stellar population is predominantly older. There is no visual evidence of a major merger or strong tidal interaction; however, some minor disturbances are plausible. No prominent bar structure is detected in the central region, but a weak bar is also not out of the question. The galaxy is observed face-on, providing a clear view of its disk structure. The galaxy's diameter suggests it is a moderate-sized galaxy.