The galaxy exhibits a generally elliptical morphology, appearing mostly smooth with a concentrated central bulge. There is a distinct color gradient, with the core appearing more yellow-orange, suggestive of an older stellar population and possibly a higher concentration of dust. Moving outward from the center, the color shifts to a bluer hue, potentially indicating a younger stellar population in the outer regions. The overall structure seems relatively undisturbed; however, subtle asymmetries or faint tidal features cannot be entirely ruled out due to the resolution of the image. The galaxy shows a clear spheroidal component with a higher degree of roundness and minimal signs of a significant disk-like structure. The outer edges fade gradually into the background, making it difficult to discern the exact extent of the galactic halo. There is no indication of significant ongoing mergers or major disturbances to its structure.
