The galaxy presents as a somewhat elongated structure. There is a central bright bulge that appears yellow to gold in color, which may indicate an older stellar population dominating this region. Fainter and bluer light extends from the central region, suggesting the presence of a disk. There is a hint of a spiral structure, but due to the resolution and distance, it is difficult to discern detailed arm morphology. The galaxy does not show obvious signs of a major merger, although minor disturbances cannot be ruled out. Overall, this galaxy appears to be relatively massive with a modest rate of star formation.
