The galaxy presents an elongated, cigar-like morphology. It exhibits a smooth texture, with a central bulge that appears more prominent along its major axis. There is a possible disk-like structure visible, but it does not present any distinct spiral arm features. The color distribution indicates a redder central region, possibly due to a concentration of older stars, while the outer regions show a hint of bluer light, potentially from younger stellar populations, even if faint. There may be subtle signs of minor gravitational disturbance, but its global structure seems to be mostly undisturbed.
