The galaxy presents an elongated, cigar-like morphology. Its light profile appears relatively smooth and diffuse, lacking prominent spiral arms or a distinct central bulge. The color gradient suggests a higher concentration of older stellar populations toward the galaxy's core, which emits light with a redder hue. The outer regions show bluer tints indicating younger stars, though these star forming regions are not well resolved. There are no obvious signs of tidal distortions or interactions with other galaxies, although the resolution is too low to rule out minor disturbances. The galaxy's shape is significantly elongated, which could either be its true form or due to viewing angle effects on a more disk-like structure. Overall, the galaxy appears to be a relatively massive system with ongoing, but perhaps diminishing, star formation.
