The galaxy presents as a flattened, disk-shaped structure, viewed at a high inclination. A prominent central bulge dominates the morphology, exhibiting a smooth, relatively featureless appearance. The disk component displays subtle color variations, with a general trend toward bluer hues at the edges and redder hues in the center, suggesting active star formation in the outer regions and an older stellar population in the core. There is little evidence of strong spiral arm structure or significant dust lanes, contributing to a more diffuse appearance. The overall luminosity profile suggests a concentration of mass towards the center, with a gradual decrease in surface brightness outwards.
