The galaxy exhibits a moderately smooth, somewhat elliptical morphology. A bright, concentrated central bulge dominates the core region, suggesting a significant population of older stars. The color of the bulge appears yellowish. Surrounding the bulge, there's a fainter, more diffuse halo or disk-like structure. The outer regions are less defined, possibly indicating a lower density of stars and gas. There is no obvious spiral structure present and there are no signs of any major disturbances indicating an ongoing merger.
