The galaxy presents as a roughly elliptical object, elongated in shape, with a smooth, seemingly featureless morphology. The light distribution indicates a concentration of older stellar populations. This is suggested by the reddish hue apparent at one end, indicative of aging stars. The opposite end displays a bluer color, hinting at the presence of more recent star formation, although this activity is not overtly prominent in the image. There is no evidence of strong spiral arms or a distinct disk structure. Minimal tidal disturbances or interactions with other galaxies are observed. The overall structure appears relatively undisturbed and stable.
