The galaxy presents a generally smooth morphology, with a slight elongation, appearing more rounded than cigar-shaped. There is faint evidence of a disk-like structure. It is also notable that there are very small, diffuse structures within the galaxy. It exhibits a distinct color gradient, transitioning from a bluer hue towards the center to a redder appearance in the outer regions. The central region displays a strong concentration of light, indicative of a possible bulge. There are no prominent signs of ongoing major mergers or significant tidal disturbances affecting the overall structure, though minor disturbances cannot be ruled out.
