The galaxy presents as a generally smooth, elliptical morphology. It exhibits a centrally concentrated brightness profile, with luminosity decreasing radially outward from the core. There is no discernible spiral structure or distinct bar feature visible in this image. The color profile suggests a relatively evolved stellar population; the central region appears slightly redder than the outer regions, possibly indicating an older stellar population and/or increased dust concentration towards the center. There is a hint of a fainter blue-ish halo surrounding the core of the galaxy. The overall structure appears relatively undisturbed, with no significant signs of tidal interactions or ongoing mergers apparent in the image.
