The galaxy presents a largely smooth, elliptical morphology with a bright, concentrated central bulge. The color gradient suggests an older stellar population dominating the central region, with a shift towards redder hues. A faint disk-like structure, elongated in shape, is perceptible with a bluer tint. Indications of disturbed morphology are minimal; suggesting that it has completed past merging events. Based on its apparent smoothness, roundness and color indices, the galaxy is relatively massive, with ongoing star formation.
