The galaxy presents as a smooth, elongated structure with an apparent cigar shape. A central bulge is visible, displaying a yellowish-white hue, suggesting a concentration of older stars. Extending outward from the bulge, a flattened disk is observed. The disk exhibits subtle color variations, transitioning from a greenish hue near the central bulge to a reddish tone toward the edges. This color gradient may indicate varying stellar populations or dust content. The overall morphology suggests an elliptical or lenticular galaxy. There is no visible evidence of spiral arms or active star formation regions, but a low level of star formation can't be ruled out. There is no indication of tidal tails or other disturbances, suggesting the galaxy is relatively undisturbed.
