The galaxy presents a generally smooth, elliptical morphology, although with some notable asymmetries suggesting possible interactions or internal disturbances. The central region exhibits a concentrated luminosity, indicative of a significant stellar population. Moving outward, the light gradually fades into a less defined halo.

The color gradients suggest a degree of complexity in stellar populations. A blueish tint can be detected in the outer reaches of the galaxy suggesting some degree of recent star formation, while the core seems to be composed of a more established population of older, redder stars. An orange tint can be observed in one region of the galaxy which is indicative of a population of evolved stars.

The galaxy's overall structure hints at a system undergoing dynamic processes. The deviations from a perfect elliptical shape and variations in color distributions suggest a complex evolutionary history, which may include minor merger events or ongoing internal activity.
