The galaxy appears as a relatively smooth, elliptical-like structure. The color profile suggests an older stellar population, with a dominant yellowish-orange hue emanating from the central region. There is a subtle color gradient, with the core exhibiting a more intense yellow compared to the outer regions, which gradually fade into a reddish tint. No distinct spiral arms or prominent dust lanes are discernible within the visible spectrum. The overall morphology indicates a system with minimal ongoing star formation. The galaxy exhibits a generally round shape, with a slight deviation that could suggest a minor tidal disturbance or the remnants of a past merger event, though it is not definitive.