The galaxy presents an elongated, cigar-shaped morphology. Its light profile appears relatively smooth, with a slight central condensation. The color distribution across the galaxy seems largely uniform, with a subtly bluer hue present throughout. There is some indication of a faint, diffuse, arm-like structure extending from one end of the galaxy. No strong evidence of a recent major merger is observed, although subtle asymmetries or minor disturbances may be present in the outer regions. Overall, the galaxy appears to be a relatively undisturbed system.
