This galaxy appears to be a relatively smooth, round structure. The light is concentrated in the central region, suggesting a bulge. The light from the bulge graduates outward. The outer regions of the galaxy are fainter than the central bulge. There's a subtle color gradient, with the central region appearing slightly more yellow-white, transitioning towards a bluer hue in the outermost regions. This color difference may be due to differing stellar populations. There's no clear evidence of spiral arms or a distinct disk. Overall, the galaxy presents as a somewhat elliptical or lenticular galaxy type. There is no evident disturbance due to interaction with another object.
