The galaxy presents as a moderately luminous system with a smooth, elliptical morphology. There is a concentrated central bulge region exhibiting a yellowish hue, suggesting an older stellar population. The outer regions display a bluer tint, potentially indicating the presence of younger stars, though star formation appears relatively quiescent. There are no prominent spiral arms or a distinct disk-like structure visible. Minor disturbances within the shape indicate a possibility of past mergers. The overall rounded appearance indicates the galaxy is approximately circular in projection.
