The galaxy presents as a spiral morphology, with a central bulge that contributes moderately to the overall light profile. The spiral arms are tightly wound, originating close to the central bulge and extending outward. A bar-like structure is evident within the bulge region, though its strength is moderate. The arm structure is complex, with a predominant two-armed pattern. The overall color suggests a mature stellar population throughout the galaxy. No signs of major mergers or significant disturbances are apparent in this image, and the disk appears relatively undisturbed, with the galaxy presenting close to face-on.
