The galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a bright, concentrated luminosity, appearing yellowish-orange in color, indicative of an older stellar population. The galaxy exhibits a slight elongation, suggesting a possible departure from a perfectly spherical shape. There is a hint of a faint disk. Faint extensions can be observed, suggesting possible interactions or tidal features, although they are subtle and not indicative of a major merger event. The color gradient transitions to a greener hue in the outer regions, which may reflect ongoing star formation activity, though it is at a low rate. The overall structure appears relatively undisturbed, indicating it is likely a stable system that is evolving at a steady pace.
