The galaxy presents a disk-like morphology with a distinct central bulge. The bulge region exhibits a concentrated luminosity, appearing roughly spherical and possessing a yellowish-white hue. The surrounding disk component shows a bluer color gradient, suggesting the presence of younger stellar populations and ongoing star formation within the spiral arms. While the galaxy appears to be relatively smooth, there are subtle indications of structural features or minor disturbances extending from the central bulge outwards. The orientation of the disk is neither perfectly face-on nor perfectly edge-on, but at a slight angle to our line of sight. There is some evidence of asymmetry in the outer regions of the galaxy, potentially due to tidal interactions or recent minor merger events. The outer regions appear fainter and more diffuse, suggesting a lower stellar density.
