The galaxy presents a generally smooth, elliptical morphology. The light profile appears concentrated towards the center, with a gradual decrease in brightness outwards. The galaxy exhibits a distinct yellow-orange color, suggesting a relatively old stellar population with fewer young, massive stars. While the overall structure is smooth, there is a subtle elongation in the shape, transitioning towards a cigar-like appearance rather than being perfectly round. There is no clear evidence of a prominent disk structure or spiral arms. Additionally, there are no significant signs of ongoing merger activity or major disturbances in its morphology. The galaxy appears relatively undisturbed.
