The galaxy exhibits a flattened, elongated morphology, appearing as a disk viewed at an oblique angle. The central region presents a bright, concentrated bulge, which dominates the overall luminosity. The bulge appears to be yellowish-white in color. Fainter, bluer, and somewhat irregular structure is observed extending outwards from the bulge, suggestive of a galactic disk with a population of younger, bluer stars or regions of star formation. The overall smoothness of the galaxy suggests it is in a relatively settled state, without major signs of recent mergers or significant tidal disturbances. However, subtle features, such as slight asymmetries, may indicate minor interactions. The galaxy appears to be relatively large and massive.
