The galaxy presents as a centrally concentrated object with a diffuse halo. The core exhibits a yellowish hue, indicative of an older stellar population. The outer regions show a slightly bluish tint, potentially suggesting the presence of some younger, hotter stars or ongoing star formation, albeit at a low rate. Overall, the galaxy appears relatively smooth, lacking prominent spiral arms or strong morphological features. There may be a subtle indication of minor tidal disturbance, or internal structure, but further analysis is needed to confirm. The morphology suggests a smooth spheroidal galaxy, possibly of an elliptical type.
