This galaxy presents a mostly smooth morphology. The central region exhibits a concentrated, bright yellowish-white hue which fades into a bluish halo. The galaxy exhibits an elongated, cigar-like shape. There is no discernible spiral structure, nor is there evidence of strong tidal disturbances, though some minor asymmetries exist. The color gradient suggests a change in stellar populations from the center outwards, where older stars are centrally concentrated in the warmer colors and the blue colors suggest younger stars at the outer regions. The galaxy does not appear to be undergoing any major merger activity, and does not appear to be a disk galaxy.