The galaxy presents as a single, relatively smooth, and rounded object. The light is concentrated towards the center, suggesting a bright, dense core or nucleus. There is a notable color gradient from the central region outwards. The core exhibits a yellow-orange hue, which gradually fades to a fainter, bluer color in the surrounding regions. There is no strong evidence of spiral arm structures or other distinct morphological features such as tidal tails or obvious distortions, implying that the galaxy is undisturbed or has undergone significant relaxation processes. The overall morphology suggests the galaxy is most likely an elliptical or lenticular type. There may be minor disturbances, but not in the form of a major merger. 
