The galaxy presents an overall elliptical morphology, appearing somewhat elongated. A central bulge is prominent and exhibits a yellowish-orange hue, suggesting an older stellar population. There appears to be a disk surrounding the bulge as well. The outer regions of the galaxy display a bluer color, which could suggest the presence of younger, hotter stars and ongoing star formation. There may be a slight tidal disturbance or merging event present in the outer disk, possibly a satellite interaction. There are no prominent dust lanes or spiral arm structures visible in this image. The galaxy shows a relatively smooth profile, with no significant irregularities readily apparent beyond the possible tidal disturbance. Overall, the galaxy is a fairly massive system in the distant Universe.
