The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a spheroidal shape. A bright, concentrated core region is visible, suggesting a high stellar density in the galactic center. The color profile indicates a redder core, possibly indicating an older stellar population. Moving outwards from the core, there's a subtle gradient towards bluer hues in the outer regions. The overall structure appears undisturbed, with no obvious signs of major mergers or tidal interactions. There may be slight disturbances in the form of asymmetric light distributions, however these disturbances are minimal. The galaxy's redshift indicates that we are observing it at a significant distance, corresponding to a lookback time of roughly 2.9 billion years. The galaxy appears to be relatively massive and is still forming stars, but at a slow rate. The color suggests that the average stellar population is relatively old.
