The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and centrally concentrated light distribution. The morphology suggests a relatively featureless structure. The color is generally uniform, with a slightly bluer hue in the core transitioning to redder colors in the outer regions. This color gradient may imply a centrally located population of younger stars or a difference in metallicity between the core and the outskirts. There is some evidence of minor disturbances or asymmetries in the outer isophotes, hinting at possible past interactions or accretion events. These disturbances are subtle, however, and the galaxy appears largely undisturbed. The galaxy shows a fairly rounded morphology, with no apparent spiral arms or a distinct disk. The isophotes are largely regular, and the overall impression is that of a relaxed and well-mixed stellar population.
