The galaxy presents as a relatively smooth, elliptical morphology, although there is some indication of a possible minor disturbance or interaction event. The core region exhibits a bright, concentrated luminosity, indicative of a high density of stars or possibly an active galactic nucleus. There is some color variation, suggesting the presence of different stellar populations within the galaxy. A central yellow-white hue implies older stars dominating the core, while a fainter blue tinge at the edges could indicate regions of more recent star formation, or a different population of stars. The overall shape is somewhat elongated, deviating from a perfectly circular form. The fuzziness of the galaxy's edges suggests a gradual decrease in stellar density, rather than a sharp boundary. There is evidence of a potential merger event, with a large mass of stars being gravitationally bound, but the individual stars appear relatively old, suggesting this merger occurred a long time ago.