The galaxy presents as a luminous, centrally concentrated object, exhibiting a smooth, elliptical morphology. A noticeable radial gradient in luminosity is observed, with the core region appearing significantly brighter and more yellow in color than the surrounding halo. The galaxy appears to be relatively isolated, showing no strong evidence of ongoing major mergers or tidal interactions. There is a faint hint of extended structure, possibly a very diffuse stellar halo, surrounding the main body of the galaxy. Patches of blue light are visible, indicating modest star formation, though these are not very pronounced.
