The galaxy presents an edge-on disk morphology. The central bulge is visibly prominent, exhibiting a rounded shape with a yellow-orange hue, suggesting a population of older stars. The disk appears thin and elongated, spanning a considerable distance relative to the bulge. There are no readily apparent signs of strong spiral arm structures. The galaxy appears relatively smooth in overall structure, with little evidence of major disturbances or active mergers. There is a slight blue hue on the left side of the galaxy, which could be from the presence of more young stars in that part of the galaxy.
