The galaxy presents as a centrally concentrated, relatively smooth object with a generally elliptical morphology. The core region is bright and appears nearly spherical. A subtle extension of the light emanates outwards from the central region, showing a hint of ellipticity. There is a general absence of distinct spiral arms or prominent dust lanes. Color gradients are present; the central regions exhibit a slightly bluer hue, which transitions to redder colors towards the outskirts of the galaxy. The overall appearance suggests an evolved system, possibly an elliptical galaxy with a low rate of current star formation. There is no apparent evidence of ongoing major mergers or significant tidal disturbances.
