The galaxy presents a largely smooth and centralized morphology. Its light profile exhibits a strong concentration towards the core, suggesting a prominent bulge component. The overall shape approximates round, though some elongation is present. The color distribution is not uniform. The central region has a yellow-orange hue, potentially indicative of an older stellar population or dust obscuration. Moving outwards from the center, the color shifts towards redder tones. Some regions surrounding the galaxy have a hint of blue, suggesting the presence of regions of more recent star formation. There is no obvious spiral structure or bar. Overall, it shows minimal signs of major disturbances or ongoing mergers.
