The galaxy presents as a relatively smooth, elliptical-like structure. Its core appears bright and concentrated, with a color gradient suggesting a slightly older stellar population concentrated centrally. There is a subtle extension or elongation. The outer regions fade gently into the background sky, with only a slight hint of a possible disk or faint, diffuse arms. The galaxy appears relatively undisturbed, lacking any major signs of ongoing merger activity or tidal interactions. Color variations within the galaxy are subtle, suggesting a well-mixed stellar population with minimal recent star formation.
