The galaxy presents as an irregular structure, with evidence of a possible ongoing or recent merger event. There are multiple luminous regions, suggesting areas of enhanced star formation activity across the body. The dominant coloration is bluish, indicative of a significant population of young, hot stars, likely concentrated in these areas. Fainter, diffuse, and redder regions are visible, and the overall light distribution is concentrated toward the center, but disturbed. The galaxy is not smooth; evidence suggests significant internal disruptions. The shape is more in-between round and elongated, as there is no clear spiral arm structure. The galaxy appears to be in a dynamic state, possibly undergoing tidal interactions or recent gravitational disturbances.
