The galaxy presents as a roughly elliptical object, with a smooth, centrally concentrated light profile. The core exhibits a distinct yellowish-orange hue, suggesting an older stellar population, potentially dominated by red giant stars. Moving outwards from the core, there is a discernible transition to a bluer color, particularly noticeable towards one edge of the galaxy. This bluer region indicates the presence of younger, hotter stars, possibly a region of ongoing or recent star formation. There is a subtle hint of asymmetry in the overall structure, which could be due to a minor gravitational interaction or internal dynamics. Based on the light distribution, the galaxy appears to be relatively evolved.
