The galaxy presents as a smooth, elongated structure. The central bulge exhibits a yellowish-orange hue, suggesting a population of older stars. Fainter, bluish-green tones extend outwards, indicating the presence of some younger stars or regions of ionized gas within the disk component. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal distortions. Its overall morphology implies an elliptical or lenticular classification, likely a galaxy with a significant spheroidal component.
