The galaxy presents as a flattened, elliptical morphology. A bright, concentrated central bulge dominates the core, exhibiting a yellowish hue, likely indicative of an older stellar population. The surrounding disk appears relatively smooth, with a gradual transition in color from the core to the outer edges. The outer regions are fainter and have a slightly bluer tint, potentially reflecting some ongoing, albeit low, level of star formation. The overall structure suggests a disk galaxy viewed at a considerable angle, approaching edge-on. No major disturbances or merging features are readily apparent.
