The galaxy presents a disk-like morphology, though the angle of observation is not perfectly edge-on nor face-on. A moderate bulge is present. Faint spiral arm structures are tentatively observable, but are not clearly defined, as the arms are not very distinct. There is a possibility of a weak bar structure spanning across the central region. No signs of major mergers or strong tidal disturbances are apparent in this image; however, subtle asymmetry in the outer disk could indicate minor interactions. The central region exhibits a yellowish hue, which is suggestive of a population of older stars. The outer regions show some bluer colors. Overall, the galaxy exhibits a relatively smooth appearance.