The galaxy presents as a luminous, relatively smooth, elliptical-like structure. The core exhibits a high degree of central concentration, radiating intensely across the visible spectrum, suggesting a significant population of older stars. There's a distinct color gradient, transitioning from a yellowish-white at the nucleus to a reddish hue in the outer regions. This color shift may indicate an evolving stellar population. Some asymmetric features suggest possible minor disturbances within the galaxy, possibly due to minor tidal interactions or mergers. A faint, diffuse halo surrounds the primary structure.
