This galaxy appears to be undergoing a major merging event. Two distinct luminous components are observed, each displaying a concentrated, elliptical morphology. The overall color profile suggests a population of older stars, with a yellow-orange hue dominating both galactic centers. Tidal features or extended arms are not prominently visible, potentially due to the advanced stage of the interaction or limitations in image resolution. The system exhibits an elongated shape, with the two components aligned along a major axis. Minimal dust obscuration is apparent, indicating a relatively clear line of sight through the merging system. Based on the image alone, it is difficult to determine the precise morphological type of the progenitor galaxies, but the lack of significant disk structures suggests they may be elliptical or lenticular galaxies in the process of coalescing.
