The galaxy appears to be an elliptical system, exhibiting a generally smooth and concentrated morphology. The light distribution suggests a centrally dominant bulge, with a radial falloff in surface brightness outwards. The color profile indicates a redder, more evolved stellar population is dominant across the galaxy. A slight ellipticity is visible, but there is little to no evidence of spiral arms, dust lanes, or other features associated with late-type or actively star-forming galaxies. The galaxy shows a high degree of central concentration. The galaxy appears isolated, lacking nearby companion galaxies or obvious signs of tidal interactions.
