The galaxy presents a somewhat elongated, elliptical morphology. Its light profile appears relatively smooth, with a concentrated central bulge that emits a bright, yellowish-white light. The outer regions of the galaxy fade in intensity, with a slight bluish tinge visible at the edges. This may suggest some level of ongoing star formation. There are no readily apparent spiral arm structures or prominent dust lanes, hinting at a more evolved or quiescent system. The galaxy shows a slight elongation, perhaps transitioning from elliptical to lenticular. There may be some minor disturbance in the overall structure. The galaxy is estimated to have an approximate diameter of just over 6 kpc.
