The galaxy presents a predominantly smooth morphology, appearing elliptical in shape. Its color profile exhibits a central concentration of light that is reddish-yellow, suggesting a population of older stars. The outskirts of the galaxy gradually fade into the background sky, indicating a decreasing stellar density with increasing radial distance from the center. There is a hint of a slight disturbance, which could point to a potential interaction with a smaller galaxy, or a minor asymmetry in the distribution of its light. No distinct spiral arm structures are visible. It's a fairly compact and dense structure, the light emitted suggests a substantial stellar mass.
