The galaxy presents a largely smooth morphology, appearing elliptical in shape. It exhibits a bright, concentrated central bulge that transitions to a fainter, diffuse halo. The color profile suggests a dominant population of older stars, with a reddish-yellow hue. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, showing no obvious signs of recent merger activity or tidal distortions. Its overall structure is consistent with a spheroid galaxy.