The galaxy presents a largely smooth and elliptical morphology. Its core appears bright and concentrated, indicative of a significant stellar population. There is a slight elongation visible, hinting that it is not perfectly spherical. The color profile exhibits a general reddening from core to outer regions, suggesting older stellar populations dominate in the periphery. Very faint hints of spiral structure are visible but do not suggest a strong spiral morphology. There is no strong evidence of on-going major merging activity, although there is some slight asymmetry in the outer halo. The galaxy appears to be in a relatively relaxed state.
