The galaxy presents as a single, relatively smooth, elliptical-like structure with a bright, concentrated core. The light emitted is mostly in the blue and green spectrum, suggesting a population of younger, hotter stars and potentially ongoing star formation. The overall morphology appears mostly undisturbed, but there's a hint of slight asymmetry, possibly indicating a minor gravitational interaction or internal disturbance. The galaxy shows a concentrated distribution of light, suggesting it is a spheroidal system with a dominant bulge component.
