The galaxy presents as an elliptical, or possibly a lenticular, morphology. The central region exhibits a bright, concentrated luminosity suggesting a substantial stellar population and potentially an active galactic nucleus, or a high concentration of stars in the central bulge. There's an observable color gradient, with the central core appearing more yellow/orange, possibly indicating an older stellar population and/or dust extinction in the core.

The outer regions of the galaxy are less well-defined, with a gradual decrease in surface brightness. It is relatively smooth in appearance, with no prominent spiral arms or dust lanes easily discernible. There might be some minor asymmetry or a very slight hint of a disk-like structure. The overall light profile is relatively smooth, indicating that the majority of the galaxy's light output is from relatively old and well distributed stars. It does not seem to be undergoing major merger events.
