The galaxy presents as a flattened, disk-like structure with a noticeable central bulge. The disk exhibits a subtle spiral arm morphology, though the arms are not sharply defined. There appears to be a slight asymmetry in the arm structure, hinting at possible gravitational interactions or internal disturbances.

The color profile suggests a mixed stellar population, with bluer regions in the disk potentially indicative of ongoing star formation and older, redder populations concentrated in the bulge. The galaxy is moderately luminous, and appears to have a considerable mass. There is no significant evidence of a major ongoing merger, though minor disturbances cannot be ruled out based on morphology.
