The galaxy exhibits a complex morphology indicative of an ongoing or recent merger event. The primary body of the galaxy appears to be relatively smooth, although with some irregular features. A prominent tidal tail or stream of material is visible extending away from the main galactic body. The color distribution across the galaxy is heterogeneous, with regions of blue light, possibly indicating active star formation, and regions of redder light, which may suggest older stellar populations or dust obscuration. There is a bright, possibly point-like source within the galaxy, suggesting the presence of an active galactic nucleus (AGN) or a bright star-forming region. The overall shape is disturbed, deviating significantly from a regular elliptical or spiral form. The galaxy appears to be in a dynamic state, likely influenced by gravitational interactions.
