This galaxy exhibits a generally smooth morphology, with a high degree of central concentration of light. The primary body of the galaxy appears largely spheroidal. Some disturbances are observed in the light distribution, implying there may be an ongoing or recent merger event occurring. Two distinct bright regions are observed within the primary spheroid, hinting that it is a major merger. The dominant color is yellowish-white, suggesting an older stellar population. Evidence of a disk structure or significant star formation regions are not readily apparent in the image. The object seems to be undergoing a major merger based on the disturbed morphology.
