The galaxy presents a generally smooth, elliptical morphology. It appears highly concentrated, with a bright, well-defined core that gradually fades into the surrounding halo. The color profile indicates a redder central region transitioning to slightly bluer hues in the outer edges. There are no clear indications of spiral arms or a prominent disk structure. The overall roundness is significant, without any noticeable elongation or signs of tidal disturbances. The light distribution is relatively uniform, suggesting an evolved stellar population with limited ongoing star formation. Based on its smooth appearance and color profile, it is likely an elliptical galaxy dominated by older stars.
