The galaxy presents as a lenticular-shaped object, with a smooth, concentrated central bulge. Its major axis is significantly longer than its minor axis. The light is dominated by a blue hue. The central bulge gradually diffuses outwards, exhibiting a faint, flattened disk structure. There is little evidence of distinct spiral arms or prominent dust lanes. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major ongoing mergers. A slight asymmetry can be seen along the major axis, suggesting a potential minor interaction or internal disturbance.
