The galaxy presents as a single, relatively smooth object with a concentrated central region. There is a slight elongation, but it is largely rounded in appearance. The color is predominantly yellowish-orange, suggesting an older stellar population with minimal ongoing star formation. There is no visible evidence of spiral arms or a defined disk structure. Minor asymmetry is observed in the outskirts, potentially indicating a past interaction or minor disturbance. The overall morphology suggests a relatively massive system.
