The galaxy presents as a concentrated central light source, surrounded by a diffuse halo. There is little evidence of spiral arm structure or a well-defined disk. The light distribution appears relatively smooth, with a slight elongation to the object's overall shape.

The central region exhibits a bluish-white hue, suggesting the presence of hot, young stars or possibly active galactic nuclei activity. Surrounding the central region, a reddish-orange tint hints at older stellar populations or dust obscuration. Minor irregularities in the outer regions may indicate some past gravitational interactions or minor disturbances in the galaxy's structure. The object's morphology is dominated by its bright, central concentration and overall smoothness.
