The galaxy appears as a central, somewhat condensed mass, with a flattened, disk-like structure. It appears to be a barred spiral galaxy, although the arms are faint and difficult to distinguish. The central bulge exhibits a brighter luminosity than the outer regions. Its color suggests a mixed population of stars, with a slight blue tint near the center, possibly indicating ongoing star formation, and redder hues in the outer regions. The disk shows some signs of disturbance or asymmetry. The overall structure is not perfectly smooth, with some irregularities visible in the disk.
