The galaxy presents as a relatively smooth, disk-like structure. Its shape appears to be in between round and cigar-shaped, with a slight elongation. There may be some subtle features or a disk visible, though it is mostly smooth in appearance. The galaxy exhibits a concentration of light in its central region, possibly indicating a bulge or a dense galactic nucleus. No strong merging features or major disturbances are observed, although very minor disturbances cannot be ruled out due to the resolution. The light profile suggests a generally old stellar population, with hints of some ongoing star formation activity implied by the galaxy's blue color. 