The galaxy presents as a slightly elongated, cigar-shaped structure with a relatively smooth appearance. There is a subtle color gradient, with a hint of bluer hues at one end transitioning towards redder tones at the other, possibly indicating differing stellar populations or dust content across the galaxy. There is no obvious spiral structure or distinct features such as star-forming regions. The galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. It could potentially have a disk-like component, but the inclination is such that this is difficult to confirm. There is a central concentration of light, potentially indicating the presence of a bulge or active galactic nucleus, though this is not definitively apparent.
