The galaxy exhibits a prominent spiral structure. Two well-defined spiral arms emanate from a moderately sized central bulge. The arms appear tightly wound near the bulge and begin to loosen further out. The arms display a mottled texture, suggesting active star formation regions distributed along their lengths. The overall color of the galaxy appears somewhat blue, indicative of a relatively young stellar population. There is no indication of a strong bar structure. There is no evidence of a major merger or strong tidal disruption. The morphology appears to be that of a relatively undisturbed spiral galaxy.