The galaxy presents as a relatively compact, elliptical or lenticular system. Its central region exhibits a bright, concentrated core, surrounded by a more diffuse halo of light. The color gradient suggests a radial variation in stellar population, with a bluer hue possibly indicating the presence of younger stars or ongoing star formation in the outer regions, contrasting with the generally redder, older stellar population expected in the core. Visual inspection reveals the disk is relatively small but distinct. Indications of a minor disturbance or interaction with another celestial object are present on the right side of the galaxy.
