The galaxy presents as a flattened, elliptical shape with a noticeable central bulge. The bulge region exhibits a yellow-white hue, suggesting an older stellar population. Surrounding the bulge is a fainter, more diffuse disk component, showing a mottled texture. A subtle blueish tint can be discerned within the disk, potentially indicative of ongoing star formation. The galaxy's overall structure appears relatively undisturbed with no obvious signs of a major merger event, however, there is a minor disturbance noted by the slight off-center concentration of an orange hued region to one side of the disk. The elongation of the galactic profile suggests it is not perfectly face-on with respect to our line of sight. The galaxy is well-resolved, allowing for some assessment of its internal structure.
