The galaxy exhibits a distinct spiral structure, with two prominent spiral arms emanating from a central bulge. These arms display a moderately wound morphology. The central bulge appears relatively small and exhibits a yellowish hue, suggesting an older stellar population. The spiral arms showcase bluer regions indicative of ongoing star formation. The galaxy's disk is the dominant feature, and it is viewed at an angle, not entirely face-on, but not edge-on either. There are no clear signs of major mergers or significant tidal disturbances, though there may be a minor asymmetry in the arm structure on one side that is worth noting. No strong bar feature is readily apparent in the central region. Overall, the galaxy presents as a classical spiral type with a moderate bulge and well-defined spiral arms.
