The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light profile. The core is a bright, concentrated region with a color index trending towards redder wavelengths. The surrounding halo exhibits a gradual decrease in surface brightness, with hints of subtle extension along the major axis. There is no apparent spiral arm structure or prominent dust lane features. The overall structure is largely undisturbed, indicating a lack of significant recent merger activity, although some minor disturbance cannot be ruled out. Overall, the galaxy appears to be a relatively quiescent system.
