The galaxy presents as a relatively smooth, elliptical-like structure with a noticeable elongation along its major axis. The central region exhibits a higher concentration of light, suggesting a prominent galactic bulge. There is a color gradient from the core towards the outer edges; the core appears to be slightly more red, and transitions to green towards the edges. Some minor irregularities or faint extensions are potentially visible, though the overall structure is largely undisturbed, with no obvious signs of a major merger event. It has an estimated effective radius of 12 kpc.
