The galaxy presents as a disk galaxy, observed at an oblique angle. The overall color appears to be a warm yellowish-orange, with a slight increase in redness in the central region. A thin, relatively faint streak of greenish-blue light appears perpendicular across the central region. The disk appears elongated, with a major axis significantly larger than the minor axis. Some subtle irregularities are visible in the disk's structure, possibly indicating minor disturbances, but it does not present as undergoing a major merger. There is a smooth, even distribution of light across the disk, suggesting an older stellar population is more dominant than the young. The galaxy is not perfectly smooth, but the presence of an ordered and well-formed structure indicates that it is not a fully irregular galaxy.