The galaxy exhibits a flattened, elliptical morphology. A concentrated, bright central bulge dominates the structure, with a gradual decrease in luminosity towards the outer regions. The disk appears relatively smooth, with a faint bluish hue suggestive of possible ongoing star formation. The overall shape is elongated, with a major axis extending roughly twice the length of the minor axis. There is a subtle asymmetry in the outer regions, possibly indicating tidal interactions or minor disturbances in the gravitational field. The overall color is indicative of a relatively evolved stellar population, with some younger, bluer stars mixed within the disk.
