The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. It exhibits a somewhat elliptical shape, appearing nearly round with a very slight elongation. The light profile suggests a higher concentration of stars and gas toward the core, which appears bright and yellowish. The outer regions display a gradual decline in luminosity, transitioning to a more subdued yellowish-red color. There are no obvious signs of spiral arms or significant dust lanes; the overall structure appears relatively undisturbed, with only hints of possible minor irregularities in the outer regions. The galaxy's light distribution is even, with no apparent signs of major mergers or tidal interactions affecting its shape, although the outer gradients show hints of possible minor distortions.
