The galaxy presents as a relatively smooth, centrally concentrated object with a diffuse, extended halo. The core exhibits a bright, yellowish hue, potentially indicative of an older stellar population. Moving outwards, the halo displays a gradual color gradient towards redder tones, suggesting the presence of evolved stars. There is no discernible spiral structure or prominent dust lanes visible in the image. The overall morphology appears elliptical or spheroidal in nature, lacking distinct features typically associated with disk galaxies. Minor irregularities or disturbances are not apparent, suggesting a relatively relaxed dynamical state.
