The galaxy presents as a relatively smooth, elliptical-like structure. The central bulge is prominent and appears more concentrated, exhibiting a yellowish hue suggestive of an older stellar population. The outer regions of the galaxy gradually fade, showing a more diffuse distribution of stars. There is no clear evidence of spiral arms or significant disk-like features. Subtle color variations are present, with the outer regions appearing slightly bluer, potentially indicating regions of recent, albeit limited, star formation. No major distortions or merging features are readily apparent, suggesting a gravitationally relaxed system experiencing minimal tidal interactions. Overall, the galaxy appears to be a mature system dominated by an aging stellar population with a low star formation rate.
