This galaxy presents as an elongated, lenticular-like structure. It appears to possess a smooth, relatively featureless morphology with a prominent bulge, indicating it is likely an early-type galaxy. The color gradient suggests a concentration of older stellar populations within the central bulge, exhibiting a yellowish hue. A fainter, bluish halo surrounds the central region, hinting at the presence of younger stars but at a low rate of star formation. The galaxy's overall structure suggests that it has likely undergone significant dynamical evolution, possibly through past mergers or interactions, resulting in its observed shape. There may be minor disturbances to its structure, but it appears to be primarily relaxed.
