The galaxy appears as a diffuse, elongated structure with a smooth overall appearance. The central region exhibits a brighter, concentrated luminosity, suggesting a higher density of stars or possibly an active galactic nucleus. The galaxy's color profile displays a subtle gradient, transitioning from a warmer, yellowish hue in the core to slightly cooler, reddish tones in the outer regions. There is no discernible spiral arm structure or dust lane obscuration visible. The galaxy exhibits a relatively undisturbed morphology.
