The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated, bright central region that gradually fades into a less defined halo. The primary color is a yellow-white hue, suggesting a relatively older stellar population. There's a subtle color gradient from the center outwards, potentially indicating some level of differential stellar distribution or dust extinction. No distinct spiral arm features are evident. The overall shape is moderately rounded, tending towards an elliptical form rather than a highly flattened disk. There's no obvious visual evidence of any major ongoing mergers or significant tidal disturbances. 
