The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge. The light distribution appears circularly symmetric. There is a noticeable color gradient, shifting from a yellow-white core towards bluer hues in the outer regions.  No distinct spiral arms or bar structures are discernible in the image. There are no other features in the image to suggest a significant ongoing merger event, although very minor disturbances may be present upon further investigation.
