The galaxy presents as a relatively smooth, centrally concentrated elliptical or lenticular system. The core region exhibits a distinct yellowish hue, indicating an older stellar population. Moving outward, a diffuse, bluer halo is observed, suggesting the presence of some younger stars, although the overall star formation activity appears to be low. The object is largely featureless; there is no apparent spiral structure, strong dust lanes, or signs of major interaction. The shape is somewhat elongated, but overall, it appears relatively relaxed and undisturbed.
