The galaxy presents a generally smooth appearance with a high degree of central concentration. Its overall color is yellowish-orange, suggesting a relatively older stellar population with fewer young, hot stars. The morphology appears elliptical, exhibiting high roundness and lacking any strong spiral arm structures or significant irregularities. There is a slight hint of a disk. No signs of major mergers or tidal disturbances are readily apparent; however, there are suggestions of minor disturbance. This galaxy likely resides at an approximate distance of 3.2 kpc.
