The galaxy exhibits a morphology suggestive of an ongoing or recent merger event. Its overall structure is disturbed and asymmetrical, with two primary luminous clumps possibly representing the cores of the merging galaxies. The northern clump displays a somewhat smoother profile with a more concentrated light distribution, while the southern clump appears less defined. The color gradients suggest a mix of stellar populations; yellower/redder tones in the core regions, and slightly bluer hues on the outskirts. Faint tidal features extending from the main body indicate gravitational interaction and disruption. The galaxy presents an intermediate spheroidal shape, not perfectly spherical, and not particularly elongated. There are some visible disturbances in the disk. A low rate of star formation is estimated.
