The galaxy presents a generally smooth and rounded appearance. The light profile appears to be relatively concentrated towards the center, with a gradual decrease in luminosity extending outward. The galaxy exhibits a yellow hue which suggests an older stellar population. There may be a slight asymmetry or minor disturbance in the galaxy's morphology with a small feature on one side. There does not appear to be any strong evidence of spiral arm structure or a prominent disk when viewed. Based on this examination, the galaxy is likely an elliptical galaxy with a significant stellar mass and modest ongoing star formation.
