The galaxy presents as a largely elliptical morphology with a smooth, concentrated central bulge. The core exhibits a bright, yellowish-white luminosity, indicative of an older stellar population. There is a subtle gradient of color moving outward from the core; faint blues, greens, and reds hint at some degree of ongoing star formation, though the overall smooth texture suggests it is not dominant. There is no clear evidence of distinct spiral arms or a well-defined disk. The galaxy appears to be isolated, showing no significant signs of tidal interactions or major disturbances in its morphology. Its shape appears mostly circular from our point of view.
