The galaxy appears as a relatively smooth, elliptical-like structure with a noticeable color gradient. The central region exhibits a strong concentration of light, with a yellowish-orange hue, suggesting an older stellar population. Moving outward from the core, the color shifts towards a slightly bluer, greenish tint. This could indicate the presence of younger stars or ongoing star formation in the outer regions, albeit at a low rate. The overall shape is somewhat elongated, but the galaxy does not appear to be highly distorted, showing no signs of a major ongoing merger. There is no clear evidence of a distinct disk structure or spiral arms; the light distribution appears relatively uniform and smooth.
