The galaxy presented here appears to be undergoing a significant merger event. Two distinct luminous regions are observed, possibly representing the cores of the original galaxies. These cores appear to be connected by a fainter bridge of material, indicative of tidal interactions and gravitational disruption. The overall morphology suggests a system that is not yet fully relaxed; it lacks a well-defined spiral structure or elliptical shape. The general shape can be defined as in between round and cigar shaped. The color suggests a significant population of older stars. The merger appears to be a major disturbance. Based on the color, ongoing star formation might be subdued, and potentially ceased completely, with a high mass.
