The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated core, suggesting the presence of a significant stellar population. The light distribution appears relatively uniform throughout the galaxy, with a gradual decrease in intensity moving outwards from the center. There is little evidence of spiral arms or distinct disk-like structures; instead, the overall structure appears spheroidal. Faint blue-ish tones are interspersed, providing evidence of younger stars. The overall color profile suggests a galaxy with a mix of stellar populations. There are no obvious signs of major disturbances or ongoing merger events. The object could be classified as an elliptical galaxy with possible recent, minor star formation.
