The galaxy presents as a generally smooth and elongated structure, possibly an elliptical or lenticular galaxy seen at an oblique angle. The central bulge is prominent, exhibiting a high surface brightness and a yellowish-white color, indicating an older stellar population. The light from the bulge gradually fades outwards, transitioning to a more diffuse, reddish halo or disk. The color suggests a lower rate of ongoing star formation and a higher concentration of older, redder stars in the outer regions. There are no obvious spiral arm features, but there could be a faint, flattened disk component. The overall morphology suggests a relatively massive galaxy that has largely exhausted its supply of gas for star formation. There are no clear signs of major mergers or tidal disturbances visible in this image.