The galaxy appears as a generally smooth, elliptical-like structure, exhibiting a high degree of central concentration. The core region presents a bright, yellowish-white hue, suggesting the presence of an older stellar population. Extending outwards from the core, a diffuse, bluer halo is observed, though the extent of discernible spiral arm structures appears minimal. There is a potential hint of minor disturbance or faint tidal features in the outer regions. The overall shape suggests a relatively relaxed system, likely an early-type galaxy, potentially at a redshift consistent with a cosmologically significant distance. The color gradients indicate a possible transition from an older, more metal-rich population in the center to a somewhat younger, bluer population in the outskirts, though the age and star formation rate cannot be decisively determined without further spectroscopic data. The galaxy does not seem to be undergoing any major merger events.
