The galaxy presents as a centrally concentrated structure with a primarily smooth morphology. There is a slight ellipticity in the overall shape, appearing somewhat oval. The core region exhibits a reddish hue, likely indicating an older stellar population. Extending outwards from the central core, a subtle transition to a greenish-blue color is observed, which may indicate the presence of a younger stellar population or ongoing star formation in the outer regions, though it is quite faint. There are no discernible spiral arms or bar structures visible within the galaxy's morphology, and there appear to be no major tidal disturbances or signs of ongoing merging events. The overall light distribution suggests the galaxy is relatively undisturbed and evolved.
