The galaxy presents as a single, relatively smooth, and concentrated object. It appears elliptical in shape, though it is difficult to determine with certainty if a disk component is present. The galaxy exhibits a color gradient, with a brighter, redder core transitioning to a slightly bluer and fainter outer region. There is no apparent indication of distinct spiral arms, bars, or active galactic nuclei features. No major disturbances or signs of an ongoing merger are visibly detectable, although some minor asymmetry is evident, perhaps hinting at a past interaction or internal dynamic process.
