The galaxy appears to be elliptical in morphology, presenting a largely smooth and featureless appearance. Its light distribution is centrally concentrated with a radial falloff in surface brightness. The galaxy exhibits a moderate degree of roundness. There is no obvious indication of spiral arms, a prominent disk, or any ongoing major merger activity. Minor disturbances or interactions might be present, but they are not strongly evident. Based on the galaxy's color and apparent smoothness, it may be comprised of an older stellar population with relatively low star formation.
