The galaxy presents as a centrally concentrated spheroid with a smooth overall appearance. The core exhibits a high surface brightness, gradually decreasing outwards into a diffuse halo. The galaxy appears to have a fairly regular elliptical morphology, with a high degree of central symmetry. There is a slight elongation. I do not observe distinct spiral arms or prominent dust lanes. The color profile suggests a population of older stars, with a yellowish-red hue dominating the central bulge. The outer regions display a bluer tint, which may indicate younger star formation. The object does not display any obvious signs of tidal distortions, major mergers, or strong interactions with nearby galaxies. There appears to be a slight disturbance.
