The galaxy presents a generally smooth morphology, exhibiting a centrally concentrated luminosity profile. The overall shape approximates an elliptical form, deviating slightly from perfect circularity. A subtle color gradient is observable, with a yellowish hue dominating the central region, suggesting an older stellar population. Progressing outward from the core, the color subtly shifts towards bluer tones, potentially indicative of younger stars forming in the outskirts, although this is not strongly pronounced. There is no clear evidence of spiral arm structures or a distinct galactic disk. Similarly, there's no obvious sign of recent or ongoing major merger events; the galaxy appears relatively undisturbed. Faint wisps are extending out from the galaxy but they are indistinct.
