The galaxy presents as a relatively smooth, centralized structure with a prominent bulge region. The core appears bright, exhibiting a yellowish-white hue, suggesting a population of older stars. A fainter, bluish disk surrounds this central bulge, indicating the presence of younger stars and potential star-forming regions. The overall shape is elliptical in nature, with hints of a flattened disk component. There may be subtle disturbances in the outer regions, though not prominent enough to suggest an ongoing major merger. It's possible this galaxy has experienced minor interaction with a smaller galaxy. Overall, this appears to be a relatively massive galaxy exhibiting moderate star formation.
