The galaxy presents a largely smooth, elliptical morphology. It exhibits a slightly elongated shape, appearing more 'in-between' round and cigar shaped. There is a subtle indication of minor disturbance, possibly hinting at tidal interactions or an ongoing merger event. Color gradients suggest the presence of a evolved stellar population. A central, bright yellowish core dominates the galaxy's light profile, likely representing an old stellar population with minimal current star formation. The outer regions appear fainter and redder in color. The relatively compact size indicates it is a galaxy with a moderate effective radius, a lower star formation rate for its mass, and likely residing at a moderate cosmological distance. 
