The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth, featureless morphology without apparent spiral arms or a prominent disk. The core region is intensely luminous, with a central concentration of light suggesting a possible nucleus. The overall color is a blend of red and blue, possibly implying a mix of stellar populations, with the red indicating older stars and the blue perhaps indicating some more recent star formation. There is no visible evidence of any tidal disturbances, major mergers, or significant interaction with neighboring galaxies. The outer regions of the galaxy fade gradually into the background, indicating a diffuse halo component.