The galaxy presents as a spiral type, with a well-defined disk structure. Multiple spiral arms emanate from the central bulge region. The spiral arms appear tightly wound. The central bulge component exhibits a moderate intensity. Several prominent star-forming regions are observed along the spiral arms, identifiable by their localized blue color. The disk exhibits an inclination relative to our line of sight, appearing closer to face-on than edge-on. There is no significant evidence of a bar structure in this image. There appears to be no indication of any major merging activity, however, there is a possibility of a minor disturbance with a slight asymmetry in one of the outer spiral arms. Overall, this galaxy presents as a relatively undisturbed, classical spiral galaxy with active star formation.
