The galaxy presents as a fairly smooth, elliptical-like structure. Its light profile suggests a high degree of central concentration, with a bright core that gradually fades into a more diffuse outer region. There is little evidence of spiral arms or distinct features. The galaxy appears largely spheroidal, displaying only a small deviation from perfect circularity. The color index seems relatively uniform across the galaxy, with a slight shift towards redder hues. There appears to be no major merger events, with no visible signs of tidal tails, distorted morphology, or interacting companions, though the presence of a possible minor disturbance cannot be completely ruled out.
