The galaxy presents as a largely featureless elliptical morphology. It exhibits a smooth, concentrated light profile, with a high degree of roundness. The core displays a yellowish hue, potentially indicating an older stellar population. Surrounding the core is a faint, diffuse halo of bluish light, suggesting the presence of some younger, hotter stars. There is no evidence of spiral arms, bars, or significant dust lanes. No indication of major merging activity or tidal disturbances is visible.
