The galaxy presents as a generally smooth, elliptical morphology. The central bulge appears bright and concentrated, with a slightly elongated shape.  There is a gradual decrease in luminosity from the core outwards, with a diffuse halo extending beyond the brighter central region. The color appears relatively uniform across the galaxy, trending towards a slightly redder hue in the inner regions, potentially indicative of an older stellar population and lower current star formation rate. There is a slight hint of asymmetry in the outer regions but it appears to be undisturbed. Overall the galaxy appears to be a relatively evolved system.
