The galaxy appears to be a relatively smooth, centrally concentrated system. There is no indication of strong spiral arm structure or a prominent disk. The light profile transitions from a bright, yellowish core to a dimmer blueish outer region. The core appears largely spheroidal, showing a high degree of symmetry. There is little evidence of ongoing major mergers or significant tidal disturbances. Faint features in the outer region suggest the possibility of minor interactions, but these are not readily apparent. The overall morphology suggests a relatively evolved system, potentially an elliptical galaxy or a lenticular galaxy seen face-on. The color gradient from yellow-white to blue might indicate a radial difference in stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars in the outer regions.
