The galaxy presents as a smooth, elliptical-like structure, with a high degree of central concentration. It is elongated, displaying a cigar-like shape. The light profile is relatively smooth without any obvious spiral arms or distinct features, suggesting it is likely an early-type galaxy. The core of the galaxy exhibits a yellowish hue, possibly indicating an older stellar population. The outer regions show a bluer color, which could indicate the existence of younger stars, or the presence of some ongoing, but subdued, star formation. There is no clear indication of a major merger event. The overall appearance suggests that this galaxy has undergone a significant period of evolution, and the shape is relatively stable.
