The galaxy presents as a primarily elliptical morphology, exhibiting a high degree of central concentration. The light is dominated by older stellar populations, evidenced by the yellowish-red hue, which is typical for galaxies with minimal ongoing star formation. The overall appearance suggests a relatively smooth, featureless structure, lacking prominent spiral arms or significant dust lanes. The lack of distinct features indicates that this galaxy may be in a relatively quiescent evolutionary state, potentially having undergone a significant merger event in the past which has since settled into a more relaxed state. The galaxy appears quite round, and does not show any significant signs of disturbance or ongoing merger activity.
