The galaxy presents a largely smooth, elliptical morphology. Its light profile exhibits a strong central concentration, with a gradual decrease in intensity towards the outer regions. The dominant color appears to be yellowish-orange in the center, suggesting an older stellar population primarily composed of red giants and dwarfs. The outer regions transition to a slightly bluer hue, potentially indicating the presence of some younger, hotter stars, although these appear to be relatively sparse. No distinct spiral arms or bar structures are visible. There are no obvious signs of recent major merger activity or significant tidal distortions in the image. The overall appearance suggests a relatively quiescent system that is in the process of winding down its star formation. The overall shape appears to be more "in-between" round and cigar shaped than distinctly round or highly elongated. Slight hints of minor disturbances can be seen on the edges of the galaxy.
