The galaxy presents a largely smooth and elliptical morphology, with a concentrated central bulge that dominates the visual appearance. The light is centrally concentrated and decreases steadily outwards. The galaxy exhibits a gradual color gradient, transitioning from a yellowish hue in the core to slightly redder colors in the outer regions, with hints of green. There appears to be minimal evidence of spiral arm structure or active star formation within the visible spectrum; this is consistent with a relatively quiescent or post-starburst stellar population. There is no apparent dust lane or significant tidal disturbance, which suggest a system that has not undergone a major merger recently, though minor disturbances cannot be ruled out. The shape is somewhat rounded, and the overall structure indicates an evolved galaxy, likely with a significant spheroidal component.
