The galaxy presents a largely smooth and rounded appearance, with a central concentration of light that fades gradually towards its outer regions. The core exhibits a warmer, yellowish hue suggesting an older stellar population. Surrounding this central region is a less concentrated area of light, displaying a faint greenish-blue tinge. The overall symmetrical structure and lack of obvious spiral arms or a prominent disk indicate a relatively relaxed morphology. There may be a minor irregularity within the outer halo, but no strong evidence of a recent major merger is evident in this image. Star formation appears to be present based on the bluer hue on the outskirts of the central core.