The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is largely elliptical or spheroidal, with a high degree of roundness. There is no apparent spiral structure, prominent disk, or signs of ongoing major merger activity. The central region appears more luminous and yellowish, suggestive of an older stellar population, whereas the outer regions exhibit a slightly bluer hue, possibly indicating some degree of younger stars or recent star formation. The presence of an older stellar population is dominant in the galaxy, but hints of new formation are there. Overall, the morphology suggests a galaxy that is relatively evolved and undisturbed.
