The galaxy appears to be a disk-type system, presented at a significant inclination to our line of sight. There is a distinct central bulge, exhibiting a yellowish-orange hue, suggesting a population of older stars. The disk component is visible, though somewhat faint and attenuated, displaying a bluish-white color at the outer edges. The disk is not uniform, with some areas appearing more diffuse than others. There is a faint red region in the disk closest to the bulge, possibly an area of dust obscuring the blue stars behind it. The overall morphology suggests a smooth light profile.
