The galaxy presents a smooth, concentrated appearance with a dominant central bulge. Its morphology suggests it is likely an elliptical galaxy or possibly a lenticular galaxy viewed face-on. The light distribution is centrally concentrated, with a noticeable falloff in intensity moving outwards. The color appears generally reddish or yellowish, consistent with an older stellar population. The galaxy shows possible evidence of interaction or merging, but the image resolution is not sufficient to confirm this with high confidence.
