The galaxy appears to be undergoing a merging event. Two distinct luminous regions are visible, suggesting the presence of two galactic nuclei in close proximity. One of the nuclei appears more spherical and concentrated, exhibiting a yellowish-orange hue. The second nucleus shows a more diffuse and elongated morphology, potentially indicating tidal distortion. A faint bridge of material may be present between the two nuclei. Overall, the system's structure is disturbed, showing evidence of gravitational interaction. The light suggests an older stellar population, with low star-formation. The galaxy appears to be relatively smooth, with the overall morphology somewhere between round and elliptical.
