The galaxy exhibits a disk-like morphology with a moderate central bulge. Prominent spiral arms are visible, displaying a medium winding pattern. The color distribution suggests active star formation regions within the arms, as indicated by bluer hues. Evidence of a possible weak bar structure is noted along the galaxy's central axis. There are potential indications of minor disturbances in the disk, possibly suggesting a minor interaction or past merger event. The overall structure appears relatively well-defined, implying it is not an advanced stage merger.
