The galaxy presents as a slightly elongated, disk-like structure, though the exact classification is uncertain due to image resolution. The central region exhibits a bright, concentrated luminosity that appears relatively smooth. Moving outward from the center, the luminosity diffuses with a distinct but faint disk visible. There is some indication of non-uniformity in the disk, but its difficult to determine if this indicates spiral arms or other disk features. The color of the central region is primarily white, with the disk showing some bluer hues. There might be faint signs of a minor disturbance or interaction, but it is hard to say for sure. The galaxy appears to be relatively isolated.
