The galaxy presents as a concentrated, elliptical-like form. The light distribution appears smooth, with no evident spiral arm structures or distinct features like prominent dust lanes or star-forming regions. The core is relatively bright, with a gradual decrease in luminosity toward the outer edges. Its color index suggests a population of older stars, potentially indicating a lower rate of star formation. There is a faint, greenish glow around the center of the galaxy. This suggests the galaxy is a relatively evolved system, possibly with a supermassive black hole at its center. Based on these features, the galaxy is likely an elliptical or lenticular type. No signs of ongoing merger events or significant tidal disturbances are visible.
