The galaxy presents a somewhat elliptical morphology, exhibiting a noticeable disk-like structure. The central bulge appears luminous and concentrated, gradually fading into the surrounding disk. The disk itself displays a relatively smooth texture. There is little evidence of well-defined spiral arms or intense star-forming regions and the inclination suggests that we are observing the galaxy at an oblique angle. The galaxy appears to be a relatively mature system, potentially transitioning toward a lenticular classification.
