The galaxy presents as a flattened, disk-like structure, viewed at an oblique angle. The central region exhibits a concentrated luminosity, suggesting a prominent galactic bulge. Moving outward from the center, the light distribution becomes more diffuse. The overall color profile indicates a mix of stellar populations, with a hint of bluer hues in the outer regions that may indicate the presence of younger stars and ongoing star formation. The outer edges of the galaxy appear relatively smooth, lacking prominent spiral arms or significant morphological disturbances. There are some subtle irregularities and slight variations in color across the disk. The structure appears to be mostly undisturbed, with no signs of major mergers or tidal interactions.
