The galaxy presents as a structured system undergoing an interaction or merger. A dominant, centrally located bulge exhibits a smooth morphology, appearing nearly spherical in shape and possessing a yellowish-white color indicative of an older stellar population.

A fainter, blue-ish component is located nearby, connected by a visible bridge of material suggesting a tidal interaction. This secondary component also appears largely smooth but with an irregular shape, likely distorted by the ongoing gravitational interaction.

The overall system exhibits a complex morphology, hinting at significant dynamical disturbance. While the main component displays a smooth appearance, the presence of a distinct secondary object with an irregular shape and the connecting tidal bridge strongly suggest a non-isolated system undergoing either a minor or major merger. This interaction likely triggers or enhances star formation activity, evidenced by the bluer colors in the secondary component.
