The galaxy presents as a spiral type, exhibiting prominent, tightly wound spiral arms that emanate from a bright central bulge. The arms display a mottled texture, suggesting active star formation regions interspersed with dust lanes. The central bulge appears smooth and concentrated, indicating a high density of older stars. The galaxy is relatively face-on, allowing for a clear view of its spiral structure. There is a bar present going through the bulge. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal interactions.
