This galaxy exhibits an elliptical morphology, appearing largely smooth and rounded in shape. A central bulge of concentrated light is evident, transitioning outward to a more diffuse halo. The color profile suggests an older stellar population, with light trending towards the redder end of the spectrum. There is little evidence of spiral arms or dust lanes. Slight distortions are possibly present, however they are not distinct and could be the result of image quality. Overall, this galaxy appears to be a relatively evolved system.
