The galaxy appears to be a relatively smooth, elliptical-like structure, exhibiting a centrally concentrated brightness profile that declines gradually with increasing radius. The core presents a yellowish hue, suggesting an older stellar population dominated by redder stars. Moving outwards from the core, the galaxy displays a transition towards bluer tones, indicating a presence of younger, hotter stars, possibly associated with ongoing or recent star formation activity. There is some minor disturbance in the morphology. Given the relative smoothness and shape, it can be classified as an early-type galaxy. The galaxy is a significant distance away, given that it is observed to have a redshift of 0.223731.
