The galaxy appears to be a flattened, disk-like structure viewed at a high inclination. This is supported by its elongated shape, resembling a cigar. A prominent central bulge is observed, exhibiting a yellowish hue indicative of an older stellar population. The disk shows a gradient of color, with bluer regions suggesting ongoing star formation. Patches of redder emission are sparsely distributed within the disk. There are no obvious signs of major disturbance or a recent merger event. Overall, the galaxy seems to be relatively undisturbed and isolated, without significant interactions with nearby galaxies.
