The galaxy presents as a spiral type, viewed at an angle between face-on and edge-on. Evident are two prominent spiral arms that emanate from a central bulge. The arms are not tightly wound, exhibiting a medium pitch angle. Star formation appears to be actively occurring within the spiral arms, as indicated by the presence of bluer regions. The central bulge is slightly elongated, potentially indicating the presence of a weak bar structure. The bulge constitutes a moderate fraction of the overall galaxy size. A minor disturbance is observed in the disk structure which could indicate a possible gravitational interaction, though not a major merger event. Overall, this galaxy presents as a somewhat typical spiral galaxy with ongoing star formation.
