The galaxy presents as a moderately luminous object with an apparent elliptical morphology. There is some indication of substructure within the galactic disc. At least two distinct color gradients are observed: a central blue-ish hue, that fades into a yellow-orange halo on the edges of the disc. The relative distribution of color suggests active star formation concentrated near the center of the galaxy. There also appears to be some indication of gravitational interaction, with possible minor disturbances. Overall, the galaxy appears to be in transition with ongoing star formation.
