The object presents as a relatively smooth galaxy with a slightly elongated, cigar-like shape. The light profile appears concentrated toward the center, indicating a central bulge component. There may be the presence of faint, diffuse spiral arm structures or extended disk features but the quality of the image is poor. The galaxy exhibits a color gradient, appearing bluer towards one end of the major axis and more yellow/red towards the other, potentially indicative of varying stellar populations or dust obscuration across the galaxy. No obvious signs of strong tidal disturbances or ongoing major merger events are apparent, although minor disturbances cannot be ruled out.
