This galaxy presents as a single, cohesive object with a relatively smooth light distribution. The morphology appears predominantly spheroidal, exhibiting a concentrated central bulge that gradually diffuses outward. There is no obvious spiral structure or distinct arms visible. The galaxy's overall shape seems close to round, without any noticeable elongation. Minor disturbances might be present but are not distinctly noticeable. The color profile shows a concentration of light toward the green spectrum, which could indicate the presence of certain active star formation or possibly ionized gas emission. The outer regions fade into the background with no clear truncation, suggesting a gradual decrease in stellar density. No signs of tidal tails or other major disturbances indicative of a recent or ongoing major merger are apparent.
