The galaxy presents as a spiral type, exhibiting a disk-like structure with a moderate inclination relative to the observer's line of sight. The central bulge is prominent and appears yellow-orange, indicating a population of older stars. Diffuse spiral arms extend outwards from the bulge. These arms exhibit a bluer hue, suggesting ongoing star formation. There is a faint bar feature crossing the bulge.

Based on the relatively smooth texture and color gradients, the galaxy appears to be in a mature stage of evolution, with neither recent major mergers nor disturbances apparent. The spiral arms are relatively tightly wound.

