The galaxy presents a generally smooth and rounded morphology. The central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus. A gradual decrease in luminosity is observed as the distance increases from the center. The overall color is a pale yellow-white, possibly indicating an older stellar population with less ongoing star formation. Faint blue-ish hues appear towards the outer regions. No distinct spiral arm structures or significant morphological disturbances are apparent. The galaxy appears relatively isolated, showing no immediate signs of tidal interactions or ongoing mergers with nearby galaxies.
