The observed galaxy exhibits a predominantly smooth morphology, though some structural features are discernible. It appears as a flattened, disk-like structure viewed at a significant inclination. The central region presents a bright, concentrated luminosity, potentially indicative of a bulge component. A distinct ring-like structure is visible around the central region. The disk shows a color gradient, trending from redder hues towards the central region to bluer colors in the outer disk. The light distribution in the outer regions of the disk is less uniform, with subtle indications of non-axisymmetric structure or faint spiral arm segments. No major merging signatures are apparent.
