The object appears as a relatively compact galaxy with a centrally concentrated morphology. The core exhibits a bright, bluish hue, suggesting the presence of a population of hot, young stars or an active galactic nucleus. Moving outwards from the center, the color shifts towards a redder hue. The galaxy exhibits some visual disturbances and a hint of asymmetry. It appears to be a single galaxy, but a potential merger cannot be ruled out entirely. The overall structure displays characteristics intermediate between a smooth elliptical galaxy and a disk galaxy with some features.
