The galaxy presents as a seemingly interacting system, possibly in the early stages of a merger event. A primary, brighter component dominates the visual appearance, appearing approximately round, exhibiting a smooth light distribution, and a somewhat concentrated core. A secondary component, less luminous and slightly elongated, is situated in close proximity to the primary component, possibly indicating gravitational interaction. There is a subtle color variation between the two galaxies, with the larger galaxy being somewhat bluer in color than the smaller galaxy, and a third feature, possibly a tidal tail, which is significantly redder than the two galaxies. The overall system shows an estimated half-light radius of a few kiloparsecs. The low specific star formation rate suggests that this galaxy could be in the process of quenching. There may be ongoing tidal effects based on its morphology, potentially triggered by the interaction.
