This galaxy presents as a relatively compact, centrally concentrated object. The core region exhibits a high degree of luminosity, appearing nearly spherical and intensely bright, likely indicating a significant concentration of stars and potentially an active galactic nucleus.

A faint, extended halo surrounds the core, displaying a subtle, irregular morphology. Some disturbances or asymmetrical features can be observed in the halo, suggesting a possible interaction or tidal influence. The color distribution across the galaxy is not uniform. The core appears relatively blue-white, while the outer regions are somewhat redder. This color gradient could indicate variations in stellar populations, with younger, hotter stars concentrated in the core and older, cooler stars dominating the outer regions.
