The galaxy presents as a relatively smooth, elliptical structure with a distinct central bulge. The overall color gradient suggests an older stellar population, with the core exhibiting a more yellow-orange hue compared to the slightly bluer periphery. The galaxy's shape is somewhat elongated, appearing closer to a cigar shape than a perfect circle. No prominent spiral arms or significant dust lanes are readily apparent. There may be faint hints of subtle disturbances in the outer regions, but these are not significant enough to classify the galaxy as undergoing a major merger or exhibiting strong tidal features. The galaxy appears relatively isolated.
