The galaxy presents as a centrally concentrated, elliptical-like system. A bright, seemingly spheroidal core dominates the luminosity profile. Moving outwards, the light gradually diminishes into a diffuse halo structure. There may be a faint hint of a disk, though it's close to face-on. No prominent spiral arms or distinct features are clearly visible. The galaxy appears relatively undisturbed, showing no clear signs of ongoing major mergers or tidal interactions. The overall color profile suggests a moderate age stellar population and mild star formation rate. There's a smooth, homogeneous appearance to the light distribution across the galaxy.
