The galaxy presents as a flattened disk structure, likely a spiral galaxy viewed at an oblique angle. A prominent central bulge exhibits a smooth, concentrated luminosity, appearing more yellow-white in color, suggesting an older stellar population. Fainter spiral arms extend outwards from the bulge; they display a somewhat patchy structure. The spiral arms present with a more greenish tint and some reddish regions, suggestive of ongoing star formation. The outer regions of the disk are considerably fainter, fading gradually into the background. The galaxy does not appear to be undergoing any major mergers or tidal disruptions based on its overall morphology. Dust lanes are subtle, but potentially present.
