The galaxy presents as a somewhat elliptical structure. It exhibits a smooth and concentrated central bulge that dominates the overall light distribution, suggestive of an older stellar population. The disk component appears faint and less pronounced, possibly containing some patchy regions that could indicate areas of ongoing, albeit low, star formation. There appears to be a color gradient from the center outwards, with the central regions appearing more yellow-red, and the outer disk showing a slightly bluer hue, implying a variation in stellar populations and/or dust content within the galaxy. There may be very minor signs of disturbance in the morphology, but it appears to mostly resemble an undisturbed galaxy.
