The galaxy appears to be in the process of a significant merger. There are three distinct nuclei, each with a slightly different color profile, indicating variations in stellar populations or dust content. The overall shape is irregular and disturbed, lacking a clear spiral or elliptical structure. There is faint evidence of tidal tails or debris extending from the central region, suggesting strong gravitational interactions. Based on the red hue of its colors, this galaxy is likely a fairly massive system with relatively low star formation activity and older stellar populations.
