This galaxy exhibits a centrally concentrated morphology with an apparent diffuse halo. The central region displays a complex structure, showing irregular light distribution. There's an indication of a possible tidal tail extending from the primary body of the galaxy, suggesting a past interaction. The core exhibits a bright, compact region potentially indicative of an active galactic nucleus or intense star formation. Broad color variation across the galaxy hints at varying stellar populations and/or dust content. The outer regions fade into the background with no clear, defined edges. There is some evidence of minor disturbances in the main galaxy body.
