The galaxy presents as a spiral type, exhibiting a disk-like structure. Prominent spiral arms are discernible, though somewhat tightly wound. A central bulge region is evident, displaying moderate size and high luminosity, which might indicate a significant population of older stars. The disk component shows a distribution of bluer regions, suggestive of active star formation. The galaxy's orientation is oblique relative to our line of sight. There is some subtle structural irregularity observable within the disk, possibly due to a minor interaction with another galaxy or internal disturbances. The overall color profile appears relatively blue, indicative of ongoing stellar formation.
