The galaxy presents an elliptical morphology, with a smooth, diffuse appearance. The central bulge region is noticeably brighter and more concentrated than the outer regions, suggesting a higher density of stars. The galaxy appears to be slightly elongated in shape, transitioning from a rounded to somewhat cigar-shaped appearance. The lack of distinct spiral arm structures or dust lanes indicates a relatively low rate of current star formation, with the overall color profile leaning towards the redder end of the spectrum. There are no apparent major merger events or significant disturbances in its overall structure. 
