The observed galaxy presents an elongated, cigar-shaped morphology. Its color profile indicates a central region that is yellowish, suggesting an older stellar population, with subtle extensions toward the edges. The galaxy exhibits a smooth appearance overall, lacking prominent spiral arms or distinct features, although faint irregular patches might be visible upon closer inspection. There is a possibility of a minor disturbance in the main shape of the galaxy, but not a full-blown merging event with another galaxy. The galaxy's light distribution gradually decreases from the center outwards.
