The galaxy presents as an elliptical morphology with a smooth, centrally concentrated light distribution. There's a noticeable radial color gradient, shifting from a more yellow/orange hue in the core to a bluer tint in the outer regions. The isophotes appear largely regular, although with some subtle deviations from perfect ellipticity. There is no obvious spiral structure or prominent dust lanes visible. The system seems relatively isolated, displaying no clear signs of major tidal interactions or ongoing mergers with nearby galaxies. The overall appearance suggests a relatively evolved system, potentially undergoing declining star formation in the core and low level of activity in the outskirts.
