The galaxy presents a disturbed morphology, indicative of an ongoing or recent merger event. The structure shows asymmetrical features, lacking a clear, defined shape. Two galactic nuclei are visible, with one appearing more diffuse and potentially further along in the merging process. The presence of prominent spiral arms are visible, with two spiral arms wrapping around one nuclei. These arms display a loose winding pattern. The galaxy appears relatively blue, suggesting active star formation within its disk and spiral arms. There are no indications of a strong bar structure. The galaxy is relatively compact in size.
