The galaxy presents a roughly elliptical morphology, though with some observable irregularities. A central, bright bulge region is evident, fading outwards into a more diffuse halo. The galaxy exhibits a generally smooth appearance, with subtle hints of possible internal structures. The overall color is primarily bluish, suggesting the presence of younger stellar populations, with subtle variations in color throughout. Some regions appear slightly redder, possibly indicating the presence of older stars or dust obscuration. There is some evidence of potential tidal disturbances or interactions, suggested by faint extensions or asymmetries in the outer halo. The isophotes appear generally smooth, though with slight distortions, supporting the presence of a disturbed system.
