The galaxy appears to be a relatively smooth, centrally concentrated system. Its morphology is primarily elliptical, with a bright, yellowish core that likely indicates a population of older stars. A diffuse, bluish halo surrounds the core, suggesting the presence of some younger, star-forming regions. There are subtle features present, indicating some level of ongoing star formation or disturbance in the disk. There is a slight asymmetry that is visible, perhaps due to a minor merging event or internal disturbances. Overall, the galaxy exhibits characteristics of an intermediate stage in its evolution, displaying features of both older and younger stellar populations.
