The galaxy appears to be a relatively smooth, elliptical-type system at a considerable distance. Its overall color is yellowish, suggesting an older stellar population with lower levels of ongoing star formation. The galaxy exhibits a centrally concentrated light profile, with a gradual decrease in brightness towards its outer regions. There is a subtle elongation in its shape, deviating slightly from perfect circularity. No distinct spiral arms or significant dust lanes are discernible in the image. There might be a very faint, diffuse halo surrounding the main body of the galaxy, but this is difficult to confirm with certainty due to the image quality. There is no obvious evidence of any major merger events or tidal disturbances affecting its structure, and no companion galaxies are apparent nearby. The galaxy's morphology suggests it has likely undergone a significant period of passive evolution.
