The galaxy presents as a generally smooth, elliptical structure with a noticeable color gradient. The central region exhibits a reddish hue, suggestive of an older stellar population or potentially dust obscuration. Moving outwards from the core, the color transitions towards a more greenish-yellow tint, implying the presence of a younger stellar population or a lower concentration of dust in the outer regions. There appears to be a slight elongation to the galaxy's shape, indicating a possible deviation from a perfect sphere. There are no clear signs of major disturbances or tidal features, suggesting it is a relatively isolated system that has not recently undergone a significant merger. Overall, the galaxy exhibits characteristics consistent with a mature elliptical galaxy with ongoing, but limited, star formation in its outer regions.
