The galaxy presents as an elliptical morphology, exhibiting a smooth, centralized luminosity profile. It appears nearly spherical, with only slight elongation. The galaxy's core is characterized by a bright, concentrated emission, indicating a high stellar density or possible active galactic nucleus. The outer regions of the galaxy show a gradual decrease in luminosity, suggesting a diminishing stellar population density with increasing radius. There are no apparent signs of spiral arms or a distinct disk component. Additionally, there are no obvious signs of a recent major merger event or tidal disturbances. There may be some low level star formation, but its small effect. It appears to be a relatively isolated galaxy.
