The galaxy presents as an object with intermediate characteristics between smooth and disk-like morphology. There is evidence of some internal structure but it is not obviously spiral. The central region appears to have higher surface brightness, transitioning outwards to fainter, diffuse regions. The overall color appears relatively uniform across the galaxy's extent, suggesting a somewhat consistent stellar population throughout, but slightly bluer toward the center, potentially indicating increased star formation or a younger stellar population within the nuclear region. There may be some degree of minor disturbance apparent in its overall shape or internal structures. There is a much smaller irregular blue object nearby that may be interacting with this object.