The galaxy presents as a somewhat oblong, smoothly distributed light source. A central bulge appears bright and concentrated, exhibiting a bluish-white hue. This color suggests active star formation within the central region. Extending outward from the core, there is a diffuse halo of light, also with a bluish tint. The morphology is suggestive of a disk galaxy, though the disk structure appears relatively smooth without prominent spiral arms. The overall smoothness may indicate that this galaxy is in a later stage of its evolution, where star formation is winding down and the spiral structure is less pronounced, or that it may be a lenticular galaxy. Faint irregularities in the outer regions hint at possible past gravitational interactions or minor disturbances.
