The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated central bulge with a noticeable radial gradient in luminosity, diminishing outwards from the core. The overall color profile suggests an older stellar population, with a yellowish-red hue dominating. There is no discernible spiral arm structure or dust lane obscuration visible at this resolution. The galaxy appears relatively undisturbed, showing no strong evidence of ongoing mergers or tidal interactions. It seems to be a fairly isolated system, exhibiting a regular, spheroidal morphology.
