The galaxy presents with a notable disk-like structure, though with some apparent distortions or irregularities suggesting possible gravitational interaction. It is characterized by a prominent central bulge, seemingly of moderate size relative to the overall disk. There is evidence of spiral arm structure, though they appear somewhat loosely wound. A central bar structure is also observable. The overall colour profile suggests a mix of stellar populations, with the bulge exhibiting a yellow-red hue indicating older stars and the disk displaying a bluer tinge indicative of ongoing star formation. There are hints of morphological disturbance, possibly due to a minor merger event. The galaxy does not appear to be perfectly symmetrical.
