The galaxy presents as an elliptical morphology, appearing somewhat flattened with an apparent axis ratio of approximately 0.7 to 0.9. Its major axis spans an approximate angular diameter of 5.5 arcseconds. There's a notable color gradient from the central bulge outwards, with a yellowish-white core transitioning into a more bluish and less luminous halo. The central region exhibits a smooth, concentrated light profile indicative of an older stellar population. Faint, diffuse outer regions suggest a gradual decline in stellar density with distance from the galactic center. No prominent spiral arm structures or dust lanes are discernible in this image. The overall appearance suggests a galaxy that is relatively evolved, with a significant fraction of its stellar mass concentrated in the bulge. There is a very subtle hint of disk-like structure, although it cannot be confirmed based on this image alone. There appears to be no major ongoing merger or tidal disturbance affecting its morphology.
