The galaxy presents as a slightly elongated, disk-like structure, viewed at an oblique angle relative to its plane. There is a distinct central bulge, which appears smooth and concentrated, and a more diffuse surrounding disk. The galaxy exhibits a color gradient from a bluer hue in the outer regions of the disk to a slightly redder tone within the central bulge. The disk shows some subtle hints of underlying structure, potentially indicating spiral arms or other features, but these are not clearly defined. There is no obvious sign of any significant ongoing merger activity or major tidal disturbances. The overall impression is of a relatively undisturbed galaxy with some ongoing star formation.