The galaxy appears as a single, largely homogenous structure. The overall color profile is relatively smooth, transitioning from a bright, yellowish core to a bluer periphery. No distinct spiral arms, bar structures, or dust lanes are readily apparent. The morphology is generally elliptical with a somewhat in between roundness. There appears to be no major disturbances to its structure, though minor gravitational interactions cannot be ruled out. The central region exhibits high luminosity, suggesting a concentration of older stellar populations. Fainter, less concentrated blue light emanates from the outskirts, indicative of some ongoing, but limited, star formation. The galaxy does not appear to be actively undergoing a major merger.
