This galaxy presents as a flattened, disk-like structure, viewed at a relatively high inclination. There is evidence of a central bulge, concentrated and bright. The surrounding disk displays a mottled texture, suggesting possible spiral arm structures. The outer regions of the disk are less defined and appear more diffuse. Some irregularities and distortions are present, hinting at potential gravitational interactions. The overall color profile indicates a mix of stellar populations, with a bluer hue in some regions of the disk and a more yellow/red hue towards the central bulge. The image also suggests low-level interactions which would support the disturbed morphology.
