The galaxy presents as a spiral type, though the arms are somewhat flocculent and lack tightly wound structure. There is a notable central bulge, which appears smooth and concentrated with a yellowish hue. The disk component surrounding the bulge exhibits a bluer color profile, hinting at ongoing star formation. Some minor distortions are visible in the spiral arm structure, indicating potential gravitational interaction with another object. A small portion of the galaxy's light appears to be scattered, with a very faint halo, indicating that the object is surrounded by a halo of stars or dust. Overall, the galaxy displays characteristics of both a relatively smooth structure and a more dynamic, actively star-forming disk, with the hint of an interaction occurring.
