The galaxy presents as an elliptical morphology, appearing largely smooth with minimal visible substructure. The central region exhibits a bright, concentrated core, potentially indicative of a supermassive black hole. Proceeding outwards from the core, the luminosity gradually decreases, displaying a diffuse halo extending beyond the central region. The color gradient suggests a population of older stars dominating the galaxy's composition. The minor disturbances fraction and merger fractions as calculated suggest that there may have been some minor merging in the past.
