The galaxy presents a somewhat amorphous, disk-like structure, though with subtle irregularities in its overall form. The central region appears relatively smooth and concentrated. The disk component is less well-defined, exhibiting some degree of patchiness and perhaps faint spiral arm segments. There may be evidence of minor tidal disturbances or ongoing mergers, as there is asymmetry visible in its shape. The color profile displays a dominant yellow-white hue in the central bulge, transitioning towards a bluer tint in the outer disk regions, suggesting regions of recent star formation. Overall, the galaxy appears to be undergoing interactions that are altering its morphology.
