The galaxy presents as an elliptical-like structure with a smooth, concentrated central bulge. There is a gradual decrease in luminosity from the core outwards, indicating a lack of distinct spiral arms or significant substructure. The galaxy displays a moderate degree of roundness. The color profile suggests an older stellar population, with a reddish hue dominating the central regions, possibly indicating a lack of significant recent star formation. There is a faint, diffused halo extending beyond the core. There may be subtle signs of tidal interactions or minor disturbances, but overall the galaxy appears relatively undisturbed.
