The galaxy presents as a luminous, ellipsoidal structure with a smooth, centrally concentrated light profile. The core region exhibits a distinct yellowish-white hue, suggestive of an older stellar population with diminished ongoing star formation. Extending outwards from the core, the galaxy displays a more diffuse, greenish-yellow halo. This halo appears relatively featureless, lacking prominent spiral arms or dust lanes. The galaxy appears to be relatively isolated and undisturbed with only minor disturbances if any. Based on the color gradients, there may be a radial decline in the age of the stellar populations, with younger stars more prevalent in the outer regions.
