The galaxy presents as a generally smooth, elliptical morphology. There is a centrally concentrated bulge exhibiting a yellowish-white color, indicating an older stellar population. The galaxy is moderately rounded in appearance. There is a slight color gradient from the core outwards, with the outer regions appearing more reddish, potentially indicating a decrease in average stellar age or increased dust extinction. There is no clear evidence of a disk structure or spiral arms. No significant tidal features or signs of recent major merger events are apparent. The overall smooth morphology suggests a relatively quiescent evolutionary history.
