This galaxy exhibits a predominantly smooth morphology with a hint of disk-like structure. Its color suggests the presence of both older stellar populations, visible in the yellow and red light, and some ongoing star formation, indicated by the blue light. The galaxy doesn't display obvious signs of a recent major merger, such as tidal tails or strong distortions, although there are some features that might suggest a minor interaction or disturbance. Overall, this galaxy appears to be a relatively quiescent system with a moderate stellar mass and a low star formation rate.
