The galaxy appears to be a relatively smooth, disk-shaped structure with a bright central bulge. Its overall color is slightly bluish, indicating the presence of some younger, hotter stars, but with a notable contribution from older stellar populations. The galaxy appears to be mostly undisturbed, and does not show any signs of tidal tails or other indications of major mergers. It exhibits a moderate level of star formation. Its roundness is somewhere between round and cigar shaped. There is a slight indication of spiral structure or a flattened disk shape, but the resolution limits a definitive classification of its spiral arm structure.