The galaxy presents a largely smooth morphology, with a dominant central bulge. The shape is generally rounded. There is a hint of a possible disk component, although it is not clearly defined. No prominent spiral arms or bar structures are visible. There is a subtle color gradient, with the central region appearing bluish, transitioning to slightly redder hues in the outer regions. This suggests a higher concentration of younger, hotter stars in the core, and a population of older, cooler stars further out. There is no obvious sign of active galactic nuclei activity, tidal tails, or other signs of recent major mergers, although there could be minor disturbances.
