The galaxy presents as a disk-shaped structure, oriented approximately edge-on relative to our line of sight. Its core exhibits a concentrated, reddish hue, suggesting a population of older stars. Progressing outward from the center, the disk appears somewhat flattened, with a mixture of yellow and orange tones indicating a mix of stellar populations. There is a slight bluing of the edge. The overall structure appears relatively undisturbed with no distinct signs of major mergers or tidal disruptions.
