The galaxy presents a largely smooth and centrally concentrated morphology. There is a subtle elongation, but overall the shape appears relatively round. The light profile suggests a gradual decrease in brightness from the core outwards, with no distinct features such as spiral arms or a bar. The color gradient is relatively uniform, trending towards slightly bluer tones in the outer regions compared to the core, indicating a potentially younger stellar population in the outskirts. There is no evidence of significant tidal disturbances, suggesting the galaxy is not currently undergoing a major merger.
