The galaxy presents as a fairly smooth, elliptical-like structure, with a concentrated central bulge. The light distribution appears relatively uniform across the galaxy, without prominent spiral arm features or distinct dust lanes visible in this image. There is a central, bright region with a yellowish hue, suggesting an older stellar population dominating the core. The outer regions of the galaxy seem to fade gradually, and have some regions of bluer color, which may suggest some ongoing star formation, although at a low rate. There is no evidence of any significant merging activity or major disturbances in the galaxy's morphology. The overall shape appears to be mostly round.
