The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central bulge exhibiting a yellow-orange hue, suggesting an older stellar population. The overall color gradient shifts from a warmer, yellowish center to cooler, bluish edges, which could be due to some presence of more recent star formation, or dust. The galaxy appears to be generally regular in shape, with no obvious signs of major tidal disturbances or ongoing mergers. There is no apparent spiral arm structure or a defined disk. The morphology is generally smooth, with a slight elongation.
