This galaxy appears to be a spiral galaxy, observed at a redshift suggesting an intermediate distance. Its core exhibits a bright, yellowish-orange hue, potentially indicating an older stellar population. The disk appears tilted relative to our line of sight. Subtle arm structures are hinted at, displaying a bluer tint compared to the central bulge, a possible sign of ongoing star formation. The overall structure suggests a relatively regular morphology, however, minor irregularities are present that could be tidal disturbances. These could indicate a past or ongoing minor merger event. Based on its physical size, the galaxy could be a large system, comparable to the Milky Way.
