The galaxy presents as a somewhat elliptical structure, displaying characteristics of a disk-like galaxy, but with a dominant, smooth bulge. Its overall color suggests a significant population of older stars, contributing to a yellowish-red hue, but it is not completely devoid of younger, bluer stars. The galaxy exhibits signs of only minor disturbances to its overall morphology, with no indications of a major ongoing merger. It is of intermediate size, and shows moderate signs of star formation.
