The galaxy exhibits a generally elliptical morphology, suggestive of an early-type galaxy. It appears to be relatively smooth in texture with a concentrated central bulge that dominates the overall light profile. Moving outwards from the central region, the light gradually decreases, transitioning into a fainter, diffuse halo. There is a slight color gradient observed, the core being more yellowish-white indicating an older stellar population. The outer regions show a faint hint of reddish tones, which could suggest the presence of dust or a slightly younger population of stars compared to the central bulge. The overall structure shows minimal signs of recent or ongoing merger events.