The galaxy presents a largely smooth, elliptical morphology. It exhibits a radial color gradient, transitioning from a bluish hue in the outer regions to a more pronounced reddish or pinkish core. The overall shape appears more oblate than spherical, leaning toward an "in between" roundness. While a central bulge is evident, there is no prominent disk structure or spiral arm morphology observable. Minor disturbances are present, although the galaxy does not appear to be undergoing a major merger. This suggests possible past interactions or internal dynamical processes. Star formation appears relatively quiescent, with no bright knots of star-forming regions easily visible. The galaxy has an estimated size of about 1.6 kpc.
