The galaxy presents a somewhat flattened, disk-like morphology. It appears face-on, or nearly so, to our line of sight. A central bulge dominates the galaxy's core, exhibiting a bright, yellowish-white hue, suggesting an older stellar population. The disk component reveals a mottled texture with hints of spiral arm structure, though the details are not sharply defined. Patches of blue scattered through the arms indicate regions of ongoing star formation. A prominent bar-shaped structure is observed across the central region of the galaxy. The overall colour profile indicates a mix of stellar populations, with the bulge containing older, redder stars, and the disk arms showing bluer, younger stars. The galaxy appears relatively isolated, with no obvious signs of major interactions or mergers.