The galaxy presents an overall elliptical morphology, appearing somewhat elongated along its major axis. The core is highly luminous and concentrated, exhibiting a yellowish-white hue indicative of an older stellar population. A distinct ring-like structure surrounds the core, displaying regions of intense, localized blue-shifted light that suggests ongoing star formation within these areas. The outer regions of the galaxy fade into a fainter, more diffuse halo characterized by a purplish color gradient. Evidence of disturbances or tidal features are somewhat apparent, with some asymmetry in the outer halo indicating the possibility of minor gravitational interactions. These features include a slight warping of the overall structure and irregular density fluctuations. The integrated light across the galaxy shows a relatively smooth profile, though the star-forming ring provides a prominent feature. The redder color index of the halo suggests a dominance of older, cooler stars in the outer regions.
