The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central region. It exhibits a somewhat spherical shape with a high degree of radial symmetry. There is no readily apparent spiral arm structure, bar, or distinct disk component. The galaxy presents a fairly uniform color profile, with a slight trend towards redder hues at the core, possibly indicating an older stellar population concentrated in the center. Faint blue or green tinges are also visible, possibly indicative of pockets of star formation, though these are minimal. There are no prominent signs of ongoing major mergers or tidal disturbances within the visible structure. The galaxy appears isolated and unperturbed based on the immediate surroundings.
