The galaxy presents a distinctly elongated, cigar-like morphology. It exhibits a smooth, relatively featureless appearance, lacking prominent spiral arms or a well-defined central bulge. The color gradient suggests a redder core region transitioning to slightly bluer hues towards the outer edges. The overall structure appears largely undisturbed, with no obvious signs of ongoing major mergers or significant tidal interactions. Given the estimated size, the light suggests it is an intermediate-mass galaxy with moderate star-formation occurring. The uniformity of the light distribution across the major axis suggests that there may be little dust obscuration along our line of sight.
