The galaxy presents as a spiral type, observed at a relatively face-on orientation. The spiral arms are discernible, with a moderate winding pattern. The arms exhibit a clumpy morphology, suggestive of active star formation regions. The central bulge appears to be of moderate size, contributing noticeably to the galaxy's overall luminosity. There is no readily apparent bar structure bisecting the central region. The overall color index suggests a relatively blue population, indicative of ongoing star formation. There is no obvious morphological evidence of a major ongoing merger event, though minor disturbances or tidal features cannot be ruled out with the current resolution. The object has a smooth overall appearance with a central point.