The galaxy exhibits a somewhat irregular morphology, appearing slightly elongated. The central region displays a high degree of luminosity, suggesting a dense concentration of stars and potentially an active galactic nucleus. The overall color gradient transitions from a bright, blue-white core to a greenish hue in the intermediate regions, with a hint of reddish colorations on the fringes. There may be some signs of minor disturbances in the outer areas. The structure suggests this galaxy has experienced some gravitational disruption, but does not display characteristics of a major merger. It may be either an elliptical or a disturbed spiral galaxy.
