The galaxy presents a disk-like structure, viewed at a slight angle to our line of sight. The central bulge is prominent and exhibits a bright, concentrated luminosity. Faint spiral arms emanate from the central region, tightly wound and somewhat flocculent in appearance. The color distribution suggests ongoing star formation, particularly in the outer regions of the disk, with bluer hues indicating younger stellar populations. The galaxy appears relatively isolated and shows no obvious signs of major interactions or disturbances.
