The galaxy exhibits an elongated, cigar-like morphology. It appears relatively smooth in the central region, with a faint, blueish-white glow suggestive of a disk-like structure viewed edge-on. A distinct redder region appears offset from the center, possibly indicating an area of dust obscuration or a region of older stellar populations. There are no obvious signs of major mergers or significant tidal disturbances. It is generally isolated within the image field. The galaxy appears relatively faint, suggestive of either a low intrinsic luminosity or significant distance.
