The galaxy presents a predominantly smooth and symmetrical morphology. There is a central concentration of light that diffuses outwards, suggesting a significant bulge component. The overall color appears to be skewed towards the redder end of the spectrum. Disk-like features appear to be largely absent, or obscured by the bulge's luminosity. There is no readily apparent evidence of spiral arm structure, which suggests a classification somewhere between an elliptical or lenticular morphology. There is no visual indication of ongoing merging activity or major disturbances in the galaxy's structure. The overall impression is one of a relatively evolved and relaxed system.