The object appears to be a spiral galaxy, seen at an oblique angle. The galaxy exhibits a noticeable disk structure with tightly wound spiral arms. There is a bright central bulge that appears relatively smooth and concentrated. The disk shows subtle color variations, with some areas appearing slightly bluer, potentially indicating regions of ongoing star formation. There is evidence of dust lanes obscuring some of the light from the bulge, which could explain the complex structure. The overall morphology appears relatively undisturbed, suggesting a fairly quiescent recent history, although a very minor disturbance might be present. The shape is in between round and cigar shaped. The estimated size suggests that this is a reasonably large galaxy.