The galaxy presents as a luminous, centrally concentrated object with an apparent elongation. It appears somewhat cigar-shaped. The central region exhibits a bright, nearly unresolved core, potentially indicating a high concentration of older stars or an active galactic nucleus. A fainter, bluer halo surrounds this core, possibly indicating ongoing star formation. There are some signs of disturbance, such as faint asymmetries in the outer regions. It is likely that the galaxy is undergoing or has undergone a minor or major merger. 
