The galaxy exhibits a complex morphology, appearing to be in a state of interaction or disturbance. A dominant, relatively circular central component is visible, exhibiting a smooth, somewhat diffuse light distribution. Extending from this central region is a distinct, elongated feature or tidal tail, suggestive of gravitational interaction. The overall shape is not strictly elliptical, showing asymmetry and irregularity. Faint luminosity is observed, suggesting that at least some part of the galaxy is in front. Evidence of a possible merger is observable with the irregular shape and extended features. More data are required to fully characterize the system and understand the nature of its interaction. 
