The galaxy presents an elliptical morphology, exhibiting a high degree of central concentration. The color profile suggests a dominant population of older stars, indicated by the yellowish-orange hue at the core. There is a subtle gradient in color temperature as one moves outwards from the central bulge; this implies a potential spread of stellar ages or metallicities within the galactic structure. A faint blue-ish halo surrounds the main body, suggesting there might be some residual star formation, but it does not contribute significantly to the overall luminosity. The galaxy appears relatively undisturbed, showing no obvious signs of recent major mergers or tidal interactions, though there is the suggestion of some minor disturbances present. The relative smoothness of the light distribution supports the classification of this galaxy as an early-type system.
