The galaxy presents as an elongated, cigar-shaped structure with a high degree of smoothness. There is a color gradient across the galaxy; the central region appears more yellow-red, indicative of older stellar populations and/or dust obscuration. The outer regions display a bluer hue, suggestive of younger, hotter stars. The galaxy does not exhibit any obvious signs of spiral arms or a prominent disk. There are no indications of major mergers or significant tidal disturbances. The galaxy appears relatively undisturbed and isolated.
