The galaxy presents as an elliptical or lenticular system, characterized by a smooth, centrally concentrated bulge with a diffuse halo. Color gradients suggest a population of older stars within the central region, exhibiting a yellowish-orange hue. The outer regions appear slightly bluer, indicating the presence of younger stellar populations or ongoing star formation, although this activity seems subdued. The overall morphology is largely undisturbed, with no prominent spiral arms or signs of major mergers. There is a slight deviation from perfect ellipticity, leaning towards an in-between shape, and minor disturbance suggesting potential past interactions. The galaxy appears relatively isolated, with no other significant galaxies in close proximity to suggest a strong ongoing interaction.
