This galaxy presents as a generally smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, suggesting a substantial stellar population. The galaxy displays a yellow-orange hue, indicating a population of older stars. There is a slight hint of green extending outside of the yellow core, suggesting on-going star formation, however, this is minimal. The roundness of the galaxy indicates minimal to no disk-like structure. There is no evidence of tidal tails or significant morphological disturbance, and the smooth structure indicates a low likelihood of recent major merger activity. The overall appearance suggests a relatively evolved system with a dominant spheroidal component.
