This galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of light, suggesting a dense core potentially dominated by an older stellar population. The galaxy's overall color appears to be red-shifted. There may be a subtle hint of a disk-like structure, but the smooth light distribution is more consistent with an elliptical classification. There is no clear indication of any major ongoing merger events or significant tidal disturbances, and the morphology appears generally undisturbed. There may be a slight amount of star formation within the galaxy. The galaxy's light distribution fades gradually from the center, indicating a smooth transition in stellar density.
