The galaxy presents as a somewhat diffuse object, elongated in shape. The light distribution suggests a relatively smooth morphology, though there are subtle variations in color and intensity across the galactic body. A brighter, reddish core is evident, possibly indicating a concentration of older stellar populations or significant dust obscuration. Some faint, elongated structure extends from the central region, hinting at the presence of spiral arms or tidal features. The overall appearance suggests a galaxy that may have experienced some gravitational interaction or internal dynamical disturbance.
