The galaxy exhibits an elliptical morphology, displaying a smooth, centrally concentrated luminosity profile. Its shape appears somewhat flattened, but not highly elongated. The light distribution decreases smoothly with radial distance from the center, lacking distinct spiral arms or other prominent features. There is a slight color gradient, with the central region appearing bluer than the outer parts, possibly indicating a population of younger stars in the core. The absence of strong dust lanes or irregular structures suggests a relatively quiescent galaxy, possibly a more evolved system. There appear to be very minor disturbances in the outer halo of the galaxy which suggest possible gravitational interactions with another galaxy at some point. The galaxy's overall appearance is consistent with an early-type galaxy undergoing minimal current star formation.
