The galaxy appears to be an elliptical galaxy, exhibiting a relatively smooth, concentrated light distribution. The central region displays a yellowish-orange hue, suggesting an older stellar population with a low rate of ongoing star formation. Moving outwards from the core, the color gradually shifts towards slightly bluer tones, although the overall color remains relatively consistent. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy appears generally round in shape, with a mild elongation. There is no obvious indication of any recent major merger events or tidal disturbances affecting the galaxy’s structure.
