The galaxy presents as an elliptical morphology, with a smooth, largely featureless appearance. The light distribution indicates a centrally concentrated bulge, fading outwards with no distinct spiral arm structures visible. Color gradients suggest a redder core, potentially indicative of an older stellar population and dust concentration, shifting to a slightly bluer hue towards the outer regions. Overall, the galaxy's form implies a system undergoing or having completed a transition toward a quiescent state. There are no signs of recent major merger events, or significant tidal disturbances. The aspect ratio suggests it's not viewed perfectly edge-on, nor face-on, but rather at an intermediate inclination.