The galaxy presents as a centrally concentrated object with a smooth, diffuse light profile, indicative of an elliptical or lenticular morphology. The galaxy core is a bright, saturated yellow-white color, likely indicating an older stellar population. There is a gradual fading in luminosity from the core outwards, with a less pronounced, diffused disk around the central bulge. The outer regions display a faint blue tint, potentially suggesting the presence of some younger, bluer stars in the outer edges or recent star formation. The galaxy shows no signs of significant tidal disturbances or major ongoing mergers. There is some indication of a minor asymmetry or warping in the outer regions on one side, possibly from a past interaction. Overall, the galaxy appears to be a relatively evolved system, possibly transitioning towards a more quiescent state, with little ongoing star formation concentrated to the outer disk.