The galaxy presents a relatively diffuse morphology. It exhibits a notable central bulge, characterized by a high surface brightness and a predominantly blue-white hue. Extending outward from the central bulge, less concentrated spiral arm structures are visible. These arms show a mottled appearance with patches of blue interspersed with darker, less luminous regions suggesting areas of active star formation and dust obscuration, respectively. There appears to be a slight distortion in the overall symmetry, possibly indicative of a minor gravitational interaction or disturbance. The outer edges of the galaxy fade into the background sky, making it difficult to ascertain the true spatial extent.
