The object presents as a spiral galaxy, viewed at an oblique angle relative to its galactic plane. The central bulge is prominent and exhibits a yellowish hue, suggestive of an older stellar population. Fainter spiral arms extend outwards. These arms display a mottled, patchy appearance, indicating regions of active star formation interspersed with areas of lower stellar density. The overall galactic disk appears slightly elongated. The presence of loosely wound spiral arms are observed. There is no obvious evidence of a strong central bar, but a hint of a weaker bar might be present. The color gradient across the galaxy suggests a transition from older stars in the bulge to younger, bluer stars in the spiral arms. No significant signs of a recent major merger event are observed.
