The galaxy appears as a single, luminous object, with a smooth, elliptical morphology. It exhibits a color gradient, appearing bluer in the central regions and gradually becoming redder towards the outer edges. This color change suggests varying stellar populations, with younger, hotter stars concentrated in the core, and older, cooler stars dominating the outskirts. The absence of distinct spiral arms or a prominent disk structure further supports the classification as an elliptical galaxy. There are no obvious signs of interaction with other galaxies.
