The galaxy presents as a moderately bright, elliptical-like structure. The core exhibits a high degree of central concentration, with a smooth transition in luminosity outwards.  A noticeable tidal tail or faint stream of material extends outward, indicating a possible past interaction or ongoing accretion event.  There appears to be a second concentration of light within this stream, separate from the primary galactic body. The galaxy color suggests an older stellar population.  The overall morphology suggests it has undergone or is undergoing some form of disturbance. The system's overall shape deviates from a perfect ellipse, further supporting the hypothesis of a past or present interaction.
