The galaxy presents as a moderately luminous object with a discernible core region exhibiting a yellowish-white hue, potentially indicative of an older stellar population. A fainter, elongated structure extends diagonally from the core. The smoother appearance of the core implies a higher concentration of stars and less ongoing star formation. The galaxy's slight asymmetry suggests a past interaction or disturbance, however there is no major disturbance. Overall, the galaxy appears relatively compact, with a smooth structure.
