The galaxy appears to be in a state of significant disturbance, exhibiting features suggesting on-going or recent merger activity. The overall morphology is neither clearly elliptical nor spiral. The central region is bright and somewhat diffuse, likely containing an active galactic nucleus. There is a pronounced asymmetry in the distribution of the galaxy's light, with irregular extensions and tidal features indicative of gravitational interactions. Faint, diffuse emission surrounds the core, extending outwards, potentially tracing remnants of the interacting galaxies. A small patch of reddish light can be seen close to the core of the galaxy. Overall, the structure hints at a complex system with potentially high star formation rates.
