The galaxy appears as a roughly elliptical structure with a notable central bulge. The core exhibits a bright, yellowish-white hue, indicating a concentration of older stellar populations. Surrounding the core is a more diffuse, bluish-green halo. This suggests the presence of ongoing star formation, possibly in a disk-like structure viewed at a shallow inclination. The galaxy's overall smoothness implies it has not undergone any recent major mergers, though there is a slight asymmetry that suggests a possible minor interaction or disturbance. Based on the color indices, the galaxy has a moderate redshift, placing it at a considerable distance.
