This galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated luminosity with a yellowish-orange hue, suggestive of an older stellar population. There is a subtle gradient in color and intensity moving outwards from the core. A slightly less concentrated and dimmer, greenish halo surrounds the center of the galaxy, indicating the possible presence of a younger, bluer stellar population or ionized gas. The overall form appears undisturbed, with no obvious signs of spiral arms or major tidal disruptions. Based on the red color in the central regions, the galaxy likely has a relatively low rate of star formation. The light distribution suggests a generally spheroidal morphology with a slight elongation.
