The galaxy exhibits a clear elliptical morphology, appearing elongated with a high aspect ratio. The central region displays a concentrated, bright core, suggestive of a higher stellar density and potentially the presence of a supermassive black hole. Moving outward from the core, the galaxy transitions to a more diffuse halo. There appears to be a slight color gradient from the center outwards. The core is reddish/yellow indicating an older stellar population, while the fainter regions surrounding the core exhibit a bluer hue, possibly indicating the presence of younger stars and active star formation. The galaxy's overall smooth appearance suggests it is a relatively evolved system with minimal signs of recent major mergers or disturbances. There is a very faint and diffuse disk.
