The galaxy presents as a spiral galaxy viewed at an angle, with an inclination that obscures a full face-on view. It exhibits a central bulge region that appears bright and somewhat concentrated, with a yellowish hue, indicative of an older stellar population. Emerging from the central bulge are spiral arms, tracing out from the core. The spiral arms exhibit a somewhat patchy appearance, suggesting regions of active star formation. There may be two main arms visible that appear tightly wound around the galaxy. The disk shows a slight blue tint indicating the presence of relatively younger stars compared to the central bulge. There is no clear sign of a strong bar structure crossing the galaxy's central region, but the appearance could be weak. The overall morphology suggests a well-defined, relatively undisturbed spiral structure.
