The galaxy presents a smooth, elliptical morphology, displaying a concentrated central bulge that fades gradually into a diffuse halo. Its overall color profile suggests a dominant population of older stars, contributing to its relatively red appearance. There's a subtle hint of bluer tones, perhaps indicating some ongoing, albeit limited, star formation within the galaxy, or residual recent star formation. No distinct spiral arm structures or prominent dust lanes are visible, confirming the overall classification of an early-type galaxy, likely an elliptical or lenticular type. The shape is moderately elongated rather than perfectly spherical. There is no indication of strong tidal interactions or recent mergers. The object appears relatively undisturbed.
