This galaxy exhibits a disk-like morphology, presented at a moderate inclination relative to our line of sight. The central bulge is prominent, appearing relatively smooth and concentrated, with a yellowish-white color, suggesting an older stellar population. A faint disk surrounds the bulge, displaying a bluer hue, possibly indicative of ongoing star formation. There appears to be some minor disturbance or asymmetry in the outer regions of the disk, perhaps due to a past interaction or accretion event. The galaxy displays a structure, though not as clearly defined, showing features that indicate recent star formation. Based on its redshift, we can classify this as a relatively distant galaxy.
