The galaxy presents a largely smooth, elliptical morphology, exhibiting a concentrated central bulge.  The overall color appears to be yellow-orange, suggesting a population of older stars with lower star formation activity. There is a slight elongation, but the galaxy is generally round in appearance.  No distinct spiral arm structures or significant dust lanes are apparent. Subtle disturbances may be present on the periphery but no clear evidence of a major merger is detected. The galaxy appears relatively undisturbed. 
