The galaxy presents a somewhat elliptical morphology, with a notable central bulge that appears relatively smooth and concentrated. The overall color gradient suggests a redder core transitioning to slightly bluer outer regions, potentially indicative of differing stellar populations. A faint, diffuse disk-like structure surrounds the central bulge, although distinct spiral arms are not readily apparent. There is a subtle asymmetry in the outer regions, possibly suggesting minor gravitational interactions or disturbances. Overall, the galaxy seems to exhibit characteristics of an intermediate-type system, possibly transitioning between elliptical and spiral morphologies. The galaxy displays low levels of star formation based on the redder color, and a moderately high mass.
