The galaxy presents as a flattened, disk-like structure, exhibiting a cigar-shaped morphology. A bright central bulge is evident, which is more luminous than the surrounding disk. The luminosity appears to diminish gradually from the core to the outer edges. The overall color gradient suggests a stellar population mix, with the core exhibiting a yellowish-white hue potentially indicating older stars, while the disk shows a bluer tint suggesting some active star formation. No pronounced spiral arms are visible. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal interactions. It has a smooth structure, with no obvious clumpy features.
