The galaxy appears as a centrally concentrated object with an overall smooth morphology. The light distribution suggests a spheroid-dominated structure, likely an elliptical galaxy or a lenticular galaxy seen face-on. The core region exhibits a brighter, yellowish hue, potentially indicative of an older stellar population. The outer regions are less defined, with a subtle fading of light intensity as you move away from the center. There is a hint of blue-ish tones in the outer regions, but it is difficult to ascertain whether these are signs of ongoing star formation or a faint disk. No distinct spiral arms or bar structures are readily apparent. There is a slight asymmetry in the outskirts, hinting at a possible minor gravitational interaction or an internal disturbance, though the overall structure remains largely undisturbed.
