The galaxy appears to be an elliptical type, exhibiting a smooth, round morphology. The light is concentrated toward the center of the galaxy, indicating a dense stellar population in the core. There is a gradual decrease in luminosity from the center outwards. The color profile suggests an older stellar population, dominated by redder wavelengths, though some bluer light appears mixed throughout. No distinct spiral arms or dust lanes are apparent. The overall impression is one of a quiescent system with little ongoing star formation and no significant interactions or disturbances.
