The galaxy presents as a flattened, disk-like structure, likely a spiral or lenticular type viewed at a moderate inclination. A central bulge is visible, appearing concentrated and possessing a yellowish hue, suggestive of an older stellar population. Surrounding the bulge is a flattened disk structure exhibiting a bluer color profile, possibly indicating the presence of younger stars and ongoing star formation. Faint, diffuse spiral arm segments can be tentatively identified within the disk, however the resolution is not high enough to make a definitive characterization. There is a slight asymmetry to the disk, with one side appearing more disturbed or extended than the other. Overall, the galaxy's morphology suggests a relatively smooth structure with a small hint of disturbance.
