The galaxy presents as a relatively compact and luminous object. It exhibits a largely smooth morphology, with a mild elongation suggesting an elliptical or lenticular classification. There is little evidence of spiral arms or significant disk structure. The galaxy's color is primarily a red-shifted yellow-orange, which could indicate a population of older stars and a relatively low rate of ongoing star formation. Subtle color variations suggest internal structure. The galaxy displays a high degree of central concentration with a gradual decrease in luminosity towards its outer edges. The object shows no obvious signs of tidal disturbances or interactions. The overall appearance suggests a well-evolved system that is in a relatively quiescent state.
