The galaxy appears as a somewhat spherical object with a smooth, diffuse morphology. The core exhibits a higher concentration of light, suggesting a central bulge component.  The overall color profile shifts from yellowish-white at the core to a slightly bluer hue in the outer regions.  No distinct spiral arms or features are readily apparent. The galaxy's smooth light distribution and lack of prominent features suggest an elliptical or lenticular classification. There is no visible evidence of any strong tidal interactions or merging activity. The color gradient indicates a potential variation in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars possibly present in the outer regions, though without more detailed data this can only be tentatively suggested.
