The galaxy presents as an elongated, cigar-shaped structure. There is a distinct central bulge that appears yellowish-orange, suggesting a population of older stars. Extending outwards from the bulge, the disk exhibits a bluer hue. There are no immediately apparent spiral arm structures. The galaxy's edges appear somewhat diffuse, fading gradually into the background, suggesting the presence of a halo. There is no obvious indication of any major mergers. Minor disturbances may be occurring, but based on the general structure the galaxy appears primarily stable.
