The galaxy presents as a flattened, elliptical morphology. The central region exhibits a high surface brightness, appearing nearly uniform in color, suggestive of an older stellar population. Moving outwards, the surface brightness decreases gradually, with the outer regions appearing fainter and less defined. The color appears to subtly redden with increasing radius from the center, potentially indicating a change in stellar population, dust content, or metallicity. There is no apparent spiral structure or any clear signs of active star formation visible in this image. The overall structure appears relatively smooth and undisturbed, indicating a more evolved system.
