The galaxy presents a clear, elongated morphology, appearing as a cigar shape in the image. There may be an indication of a bulge at one end along its major axis, and a faint, diffuse tail or disk-like structure extending from the opposite end, suggesting a possible interaction or past merger event. The galaxy displays a color gradient along its length, transitioning from a bluer hue at one end to a redder hue at the other. The bluer region potentially indicates a higher concentration of younger, hotter stars and ongoing star formation, while the redder region might suggest an older stellar population. There's no obvious indication of distinct spiral arms or a barred structure. Overall, this galaxy appears to be a relatively undisturbed system that is slowly evolving, but the asymmetry and color gradient warrant further investigation into its formation history.
