The galaxy appears to be undergoing a major merger. The object exhibits a disturbed morphology, with two distinct, bright nuclei visible. A faint, diffuse halo surrounds the central region, suggesting tidal interactions between the merging galaxies. The overall color is dominated by a yellowish-white hue, possibly indicating an older stellar population, though there are also areas of blue hinting at younger stars. There are notable disturbances, with luminous clumps likely representing regions of active star formation triggered by the merger. The shape is distorted, far from a regular elliptical or spiral form. There is an overall oblong shape with a smooth appearance, indicating that it is not spiral.
