This galaxy presents as a somewhat elliptical structure, appearing relatively compact. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars or potentially an active galactic nucleus. Surrounding the core is a fainter, more diffuse halo. The outer regions display subtle, irregular features that might indicate tidal interactions or past merger events. There are hints of slight disturbances in the shape of the galaxy, particularly in the periphery, but no major disruptions are apparent. The overall color suggests a diverse stellar population, with a notable presence of older, redder stars alongside younger, bluer stars in the inner region.
