The galaxy presents a distinct spiral structure with well-defined arms. These arms are prominent and extend outwards from a central bulge. The bulge appears moderately sized relative to the overall galaxy. There's a hint of a bar-like structure crossing the bulge. The spiral arms exhibit varying degrees of density and are traced by regions of active star formation. There is no indication of significant tidal disruption or a major merger event, although there could be some minor disturbance. Based on the tightness of the spiral arms and the prominence of the bulge, it is likely an intermediate spiral galaxy. The disk is viewed face-on and appears moderately inclined relative to the observer's line of sight.
