The galaxy presents as a somewhat featureless, elliptical morphology. Its color profile exhibits a central concentration that is yellowish-white, transitioning to a more orange-red hue in the outer regions. This color gradient suggests an older stellar population dominating the central bulge, with a potential presence of younger, bluer stars in the periphery. The galaxy's overall structure appears largely undisturbed, without any obvious signs of recent major mergers or tidal interactions. The light distribution is smooth, further supporting the classification as an elliptical galaxy, with limited indication of spiral arms or significant dust lanes.
