The galaxy presents as a roughly elliptical-shaped object. The light distribution appears relatively smooth and centrally concentrated, with a bright core. The outer regions exhibit a gradual decline in luminosity without any distinct spiral arm structures readily apparent. The overall color profile suggests a relatively evolved stellar population, with a yellowish-red hue predominating. There is only a slight hint of blue. A degree of asymmetry is observed in the outer isophotes, possibly indicative of a minor tidal disturbance or past interaction. Evidence of ongoing major merger activity or significant star formation regions is absent based on the imaging data.
