This galaxy presents as a luminous, elliptical-like structure with a generally smooth morphology. The central region exhibits a bright, concentrated core, possibly indicative of a supermassive black hole or a dense stellar population. Moving outward from the core, the luminosity gradually decreases, forming an extended halo. The overall color appears somewhat red, suggesting a population of older stars. There is no obvious spiral arm structure or significant dust lanes visible, further supporting its classification as an elliptical galaxy. Minor asymmetries or subtle features might be present, but these appear minimal, and there is no evidence of major mergers or tidal disturbances. The galaxy displays an intermediate degree of ellipticity, appearing neither perfectly spherical nor highly elongated.
