The galaxy presents as a relatively smooth, elliptical structure, though with some apparent disky features. It appears oblong, significantly longer than it is wide. There is a noticeable color gradient, with a bright, yellowish core suggestive of an older stellar population. This core gradually fades into a bluer, less intense outer region. The blue tint indicates the presence of younger, hotter stars, suggesting ongoing star formation at a moderate rate within the galactic disk. The overall morphology suggests minimal recent or ongoing mergers or significant disturbances. The galaxy is a relatively massive system, emitting significant light at a redshift consistent with a moderate cosmological distance.
