The galaxy presents as a merger in progress. Two distinct nuclei are visible, both exhibiting a reddish hue indicative of an older stellar population. A diffuse halo of material surrounds both nuclei, with a yellowish-green tint suggesting a mix of stellar populations and potentially ongoing star formation. The overall morphology is disturbed, lacking a clear disk or spiral structure. Tidal features appear to be present, though the image resolution limits definitive identification. The galaxy's roundness is not immediately obvious but is most likely an intermediate oval shape. Evidence of a major merger is very apparent. The overall luminosity is relatively high, hinting at a substantial stellar mass.
