The galaxy presents as a spiral galaxy, inclined relative to our line of sight. Two well-defined spiral arms extend from the central bulge. The arms are somewhat tightly wound. The spiral arms appear asymmetric, potentially indicating a minor gravitational disturbance. The central bulge appears yellowish-white, suggesting a population of older stars. The spiral arms display a bluer hue, indicative of ongoing star formation. No strong bar structure is obviously visible. The disk appears dominant. There are no strong signs of a major merger or merging event but a potential minor disturbance.