The galaxy appears as a slightly elliptical, disk-shaped structure with a prominent central bulge. The bulge exhibits a smooth, concentrated light profile, suggesting an older stellar population. The disk component, while present, lacks defined spiral arms or significant star-forming regions. The color profile indicates a gradual transition from the yellower central bulge to a slightly bluer, but still relatively subdued, disk. The overall morphology is consistent with a relatively evolved galaxy, possibly undergoing a transition from a spiral to a lenticular type, though this is difficult to determine from the image alone. There may be some minor disturbances in the disk structure, hinting at potential past interactions, however the morphology is largely undisturbed.
