The object presents as a relatively compact galaxy, approximately elliptical in appearance. A bright, concentrated central region dominates, suggesting a significant stellar density at the core. The luminosity decreases noticeably from the center outwards, with a faint, diffuse halo extending beyond the main body. A slight asymmetry or minor perturbation is perceptible in the outer regions of the galaxy, possibly indicating an interaction or disturbance. The color profile appears consistent across the galaxy, showing a slight blueness in the center and in the outer edges. The object does not show any spiral arm structure or an obvious disk component within the image resolution.
