The galaxy exhibits a morphology that suggests an ongoing or recent merger event. Its overall shape is irregular, displaying a disturbed and elongated profile. One component appears to be a relatively smooth central region, while the other is more diffuse and distorted. There is an indication of tidal features or debris extending from the galaxy, possibly indicating gravitational interactions. The color distribution seems to be uneven, with some regions showing bluer tints and others displaying redder colors. This may suggest variations in stellar populations or dust content.
