The galaxy presents as a centrally concentrated object with a smooth light distribution. It is elliptical or lenticular in shape. The core is a bright yellowish color, suggesting an older stellar population dominating the central region. The outer regions are fainter and show a slight reddish tint. There is little evidence of spiral arms or significant dust lanes. Overall, it appears to be a relatively evolved galaxy, possibly with ongoing, but low, levels of star formation. No strong signs of recent mergers or tidal disturbances are visible. The color gradient from the core to the outer regions suggests a radial variation in stellar populations, where the younger populations inhabit the outer region of the galaxy.
