The galaxy appears to be a spiral galaxy, exhibiting a disk-like structure. Spiral arms are clearly visible, characterized by tightly wound morphology. A central bulge is prominent, displaying a moderate size relative to the overall galactic structure. Dust lanes are faintly discernible within the spiral arms, contributing to the galaxy's overall texture. There may be a slight warp to the disk, but it is difficult to tell from this angle. There is no evidence of a strong bar feature in the galactic center. Star formation appears evident within the spiral arms, as suggested by the presence of bluer, more luminous regions. The galaxy doesn't appear to be undergoing any major mergers or disturbances, based on the relatively undisturbed structure. Overall, the galaxy presents a well-defined spiral structure with indications of ongoing star formation.
