The galaxy presents an overall elliptical morphology, appearing mostly smooth in structure. There is a slight elongation visible, indicating a deviation from perfect circularity. The central region exhibits a higher surface brightness, likely indicative of a dense stellar population or active galactic nucleus. A faint, diffuse halo surrounds the core, gradually fading into the background sky. The color appears relatively uniform across the galaxy, with a subtle shift towards redder hues. There might be some subtle disturbance or tidal feature visible along the galaxy's edges, but it is difficult to tell without further analysis. The galaxy's shape implies a moderate degree of internal rotation or anisotropy in its stellar orbits.
