The galaxy presents an elliptical morphology, elongated along its major axis. The central region exhibits a concentrated, reddish hue, possibly indicative of an older stellar population or dust obscuration. Surrounding this core is a more diffuse, greenish area, which might suggest ongoing star formation. The outer regions fade into a bluish halo, indicative of younger stars. There may be some irregularities visible in the disk, possibly signaling minor disturbances. Overall, the galaxy appears relatively smooth in structure, without strong indications of spiral arms.
