The galaxy presents as a spiral type, exhibiting a well-defined disk structure. The central bulge appears prominent and exhibits a yellowish hue, indicative of an older stellar population. The spiral arms are tightly wound and are populated by what appears to be distinct star-forming regions, exhibiting a bluer color. Dust lanes are observed within the arms, contributing to the somewhat patchy appearance of the disk. The overall orientation of the galaxy is inclined relative to our line of sight. The galaxy appears relatively isolated.
