The galaxy presents a disk-like morphology with a prominent central bulge. Spiral arms are visible, exhibiting a somewhat flocculent structure. The spiral arms have a moderate winding, appearing neither tightly wound nor loosely defined. Two dominant spiral arms are visible. Evidence of an internal bar is present, possibly a weak bar structure bisecting the bulge. The galaxy exhibits a complex morphology with no major merger currently occurring, but there are signs of minor disturbance, likely interactions, that could influence the stellar distribution and gas dynamics within the galactic disk. The bulge size seems moderate. Star formation appears to be occurring within the disk and spiral arms, although not intensely.
