The galaxy appears to be a luminous elliptical type, exhibiting a smooth, symmetrical morphology with a high degree of central concentration. The color profile indicates a population of older stars, as evidenced by the yellowish-red hue dominating the central region, transitioning to a slightly bluer, but still relatively subdued, halo. There is no discernible spiral arm structure or dust lane obscuration visible. The overall roundness suggests minimal rotational support. Any ongoing star formation is likely occurring at a very low rate, evidenced by the lack of bright blue star-forming regions. There is no strong evidence of any major ongoing merger activity.
