The observed galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in shape. The light distribution is concentrated towards the center, exhibiting a strong, bright, and yellowish core, indicative of an older stellar population. This concentration diminishes outwards, transitioning into a redder halo. There is no apparent spiral structure or active star formation regions visible. The galaxy appears relatively undisturbed, showing no signs of major merging events or significant tidal distortions, however, there could be minor disturbances. The overall color suggests a relatively passive galaxy with minimal ongoing star formation.
