The galaxy appears to be in the late stages of a merger event. Two distinct luminous components are visible, potentially representing the nuclei of the progenitor galaxies. The main body displays a somewhat irregular, elongated shape, deviating from a simple elliptical or spiral morphology. There's an extended, diffuse halo of light surrounding the primary components, suggestive of tidal debris or a disturbed stellar population resulting from gravitational interactions. It exhibits a yellowish hue overall, which hints at an older stellar population dominating its light emission. One bright region to the upper left exhibits a slightly bluer hue than the rest of the object and may be evidence of a more recent star formation region. The presence of tidal tails or prominent shells is not immediately apparent in this image, although the extended halo suggests a disturbed structure.
