The observed galaxy presents as a spiral type, exhibiting a disk-like structure. There is evidence of well-defined spiral arms, tightly wound and extending outwards from a central bulge. The bulge appears small relative to the disk, and its color suggests an older stellar population. Star formation appears active within the spiral arms, as indicated by the patchy, bluish regions. No signs of a strong bar structure are apparent. There may be signs of a weak bar. The galaxy shows no obvious signs of interactions or major mergers, appearing relatively undisturbed.
