The galaxy presents a flattened, disk-like morphology, viewed at a high inclination relative to our line of sight, approaching edge-on. The central region exhibits a concentrated, brighter profile, suggesting the presence of a bulge. The overall color appears bluish-white, potentially indicative of ongoing or recent star formation, although the color is less saturated suggesting the presence of older stars as well. There are some irregularities present in the galaxy that may represent minor disturbances, or the beginning stages of a galactic merger.
