The galaxy presents as a spiral type, exhibiting a prominent central bulge that appears largely spheroidal and emits a strong, concentrated light. Surrounding the bulge, distinct spiral arms are observed. These arms are tightly wound, displaying a continuous pattern around the galaxy. The color of the spiral arms suggests active star formation regions, characterized by a bluer hue compared to the yellowish-white bulge. The disk of the galaxy appears relatively undisturbed, showing no strong indications of recent major merging events or tidal disruptions. The galaxy is viewed at a slight angle, with its disk oriented close to face-on. Faint dust lanes are subtly visible, interwoven within the spiral arms, adding to the complexity of the galaxy's structure.
