The galaxy presents as a disk-shaped structure, viewed at an oblique angle, somewhere between face-on and edge-on. A central bulge is apparent, exhibiting a bright, concentrated luminosity. The outer regions of the galactic disk display a more diffuse, less concentrated light distribution. The color profile suggests a presence of older stellar populations in the central bulge, indicated by the yellowish hue. The disk shows a mixed population, with some hints of bluer regions possibly indicative of ongoing or recent star formation. The outer edges of the disk are not sharply defined, gradually fading into the background sky. There is some indication of possible disturbance or interaction in the disk structure, as there is a very slight asymmetry.
