The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a noticeable color gradient, transitioning from a more yellowish central region to a bluer outer periphery. There is some indication of a very slight elongation, however the galaxy is mostly round in shape. The overall appearance suggests an older stellar population dominating the central region, with possible ongoing, but low, levels of star formation occurring in the outer regions. There may be evidence of some minor gravitational disturbance, possibly due to a past minor merger event. The lack of distinct spiral arms or a prominent disk suggests a classification leaning towards early-type galaxy morphology.
