The galaxy presents a largely smooth and elliptical morphology. The color profile suggests a population of older stars, with a dominant yellowish-orange hue. There is little to no indication of spiral arms or distinct features, such as dust lanes. The overall round appearance suggests a low degree of rotational support. There's no obvious ongoing major merger events or tidal disruptions visible within the galaxy's structure. The apparent lack of blue colors implies low levels of current star formation. The galaxy appears fairly isolated, with no indications of strong gravitational interactions with nearby galaxies.
