The galaxy presents as a somewhat rounded, single object in the image. Its light profile appears relatively smooth, with a concentrated central region that gradually fades outward. There is a suggestion of minor asymmetry or a possible disturbance in its structure, potentially indicating an interaction or merger event. The galaxy displays a yellowish-orange hue, which could imply an older stellar population with less ongoing star formation. Given the smoothness and color, this galaxy might be classified as an elliptical or S0 type galaxy.
