The galaxy presents with a central bulge that appears somewhat diffuse, exhibiting a yellowish-white hue. It appears disk-like, but it is unclear if the arms are spiral or irregular. There is slight evidence of possible tidal disturbances with asymmetric features extending from the main galactic body. A minor merger event or internal dynamic instability may explain these features. The outer regions display a bluer color profile in relation to the center bulge. The galaxy's overall structure suggests a transition stage, potentially between an elliptical and a spiral morphology, or a spiral that has undergone a merger event.
