The galaxy presents as a moderately compact object with an elliptical morphology. It exhibits a smooth, centrally concentrated light profile with no immediately apparent spiral arm structures or prominent dust lanes. The galaxy's color index suggests a population of relatively old stars, with a redder overall hue. The object's elongated shape indicates it is not perfectly spherical and shows some degree of flattening. There is no evidence of ongoing major merger activity, although subtle disturbances cannot be ruled out. The size appears relatively modest, suggesting that it is either a dwarf elliptical galaxy or a more massive elliptical at a significant distance.
