The galaxy presents as a disc-shaped structure viewed at an oblique angle. The central region exhibits a smooth, concentrated luminosity profile, suggesting a bulge component. Surrounding the bulge, a fainter, extended disc is apparent, displaying some subtle structural features. The color distribution appears relatively uniform, with a slight reddening towards the central regions, indicative of potentially older stellar populations or dust obscuration. There's a suggestion of some asymmetry or possible tidal disturbance on one side of the galaxy, perhaps resulting from a minor interaction. The morphology is somewhere between smooth and clearly featured.
