The galaxy presents as a flattened elliptical shape, appearing relatively smooth and homogenous in structure. A concentrated central bulge exhibits a yellowish hue, suggesting an older stellar population dominated by evolved stars. Moving outward from the center, the color subtly shifts towards a redder, but still relatively uniform distribution, indicating a possible decline in star formation activity towards the galactic periphery. There's no clear evidence of spiral arms or significant dust lanes within the visible light spectrum. The overall morphology implies a galaxy that is relatively evolved with a quiescent star formation rate. The overall shape suggests that it is not undergoing any major merging events, as its structure is largely undisturbed. 
