The galaxy appears as a centrally concentrated, elliptical-like object with a smooth, diffuse halo. The core exhibits a yellowish-orange hue, suggesting a population of older stars dominating the central region. The light gradually fades towards the outer edges of the galaxy, and there is a hint of bluer colors further away from the core, implying a presence of younger stars that might be forming. There are no distinct spiral arms or strong indications of active galactic nuclei. There appear to be no major distortions or tidal features suggestive of recent major merger events, though minor disturbances cannot be ruled out. The overall morphology points toward a relatively quiescent galaxy with a predominantly evolved stellar population.
