The galaxy presents an elliptical morphology, though with hints of a possible disk component viewed nearly edge-on. The central bulge appears relatively prominent and displays a yellow-red hue, possibly indicating an older stellar population. Extending outward from the bulge, a faint, elongated structure is visible, suggesting a disk. This disk shows some blue-green color, hinting at the presence of younger, hotter stars and active star formation regions. The galaxy lacks a strong spiral arm structure and appears fairly smooth. There is a slight asymmetry or minor perturbation in the disk's outer regions, suggestive of a possible past interaction or minor disturbance. The overall shape is somewhere between round and elongated cigar-shaped.
