The galaxy appears to be an elliptical galaxy at a considerable distance, exhibiting a smooth, symmetrical morphology. It has a generally round shape, with a high degree of central concentration of light, indicating an older stellar population. There is a gradient in color towards the center, where it appears more yellowish, potentially due to the presence of older, redder stars. There is no apparent spiral structure or disk-like features, and no obvious signs of recent merger activity or significant tidal disturbances. The galaxy appears relatively isolated, without any nearby companion galaxies distorting its shape. The galaxy is fairly compact, with a small angular size. Overall, it presents as a relatively quiescent system with little ongoing star formation.
