The galaxy presents as a centrally concentrated object with a smooth, somewhat elliptical morphology. There is a slight elongation along one axis, but the object is generally rounded in appearance. The central region appears brighter and more compact than the surrounding area, suggesting a higher concentration of stars and potentially a bulge. There are subtle color gradients, with the central region exhibiting a yellowish-white hue, transitioning to a bluish tinge in the outer regions. No distinct spiral arms or prominent dust lanes are visible. There is a subtle irregularity visible, which may or may not indicate a potential minor interaction. Overall, the galaxy appears to be a relatively evolved system with ongoing star formation, but not at a significant rate.
