The galaxy presents as a roughly elliptical form, displaying a largely smooth morphology. The central region exhibits a concentrated luminosity, appearing significantly brighter and more yellow/gold in color than the outer regions, suggesting a possible population of older stars and minimal ongoing star formation within the core. Moving outwards from the central bulge, the color appears slightly bluer, possibly indicating the presence of a younger stellar population. The galaxy seems relatively undisturbed, without any obvious signs of major mergers or tidal disruptions, although a slight asymmetry or minor disturbance is possible in the outer edges. There's a small area that appears more red, indicating a region with greater dust obscuration or more older stars. Overall, the galaxy shows a general symmetry characteristic of an early-type galaxy, transitioning towards a less luminous halo.
