This galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated morphology. The galaxy's light profile suggests a centrally concentrated bulge, with a gradual decrease in luminosity outward. The color gradient suggests an older stellar population, as the central region appears more yellow than the bluer outer regions. No distinct spiral arms or significant dust lanes are apparent. The galaxy displays an apparent round shape. There is no obvious visual evidence of a major ongoing merger, though subtle irregularities in the outer envelope cannot be completely ruled out as minor disturbances. Overall, the galaxy presents as a relatively quiescent system.
