The galaxy appears as a singular, concentrated object. Its overall morphology suggests a predominantly smooth structure, with minimal discernible features such as spiral arms or a prominent disk. It exhibits a nearly round shape in its overall form, showing little deviation towards an elongated or cigar-like appearance. There is no obvious presence of any major mergers occurring, with no stark visual signs of tidal tails, double nuclei, or significantly distorted structures. The light profile appears relatively consistent, lacking the clumpy or irregular patches which are common in merging systems. The color suggests it has intermediate star formation properties and moderate mass, and it is a singular object in space.
