The galaxy presents as a relatively smooth object with an elliptical morphology. The central region exhibits a high degree of luminosity, with a gradual decrease in intensity towards the outer edges. There appears to be a subtle disk-like structure present; however, distinct spiral arms are not evident within the observed features. The overall color suggests a lack of significant recent star formation, with the dominant stellar population likely composed of older, redder stars. Minor disturbances may be apparent in the outer regions, although no major merging events or significant tidal distortions are observed. The galaxy is roughly round, with a small population possibly undergoing interactions.
