The galaxy presents a predominantly smooth morphology. It appears nearly circular in shape, with a high degree of roundness. The galaxy's light profile suggests a centralized concentration, typical of early-type galaxies. A slight color gradient is noticeable; the central region exhibits a bluish-white hue, transitioning towards a redder shade in the outer regions. The image suggests ongoing, albeit moderate, star formation. There is some evidence of tidal disturbances, as seen through the faint asymmetry on the left side of the galaxy, indicating a possible interaction or past merger event, potentially involving a smaller system nearby.