The galaxy presents as a slightly elongated, disc-like structure. The central bulge exhibits a strong concentration of light, appearing a yellow-white hue suggesting an older stellar population. The disk itself shows a bluer color profile, hinting at the presence of ongoing star formation. The galaxy appears relatively smooth and without prominent spiral arms. The disk is not perfectly circular, displaying a subtle cigar-shaped morphology. There is no evidence of any major mergers or tidal disturbances in this image.
