The galaxy presents a lenticular morphology, appearing as a smooth, flattened disk when viewed from our perspective. It exhibits a central bulge that is brighter and more concentrated than the surrounding disk, giving it a yellowish orange coloration. The disk component appears relatively featureless, lacking prominent spiral arm structures. There is a slight elongation noticeable across its major axis, giving it a cigar-like shape. Evidence suggests that there is minimal to no on-going major merging events. The galaxy appears to be red-shifted, indicating considerable distance.
