The galaxy appears as a somewhat smooth, centrally concentrated object. There is a subtle elongation, deviating slightly from a perfect circular shape. The light is predominantly yellow-orange, suggesting a population of older stars. A small fraction of blue light is observed near the center of the galaxy, hinting at a small population of younger, hotter stars or a weakly active galactic nucleus. The overall structure lacks prominent spiral arms or a distinct disk; it seems to be dominated by a bulge component. There are some signs of minor disturbances in the morphology but there is no strong sign of it undergoing a major merger, as the image shows a somewhat even light distribution. The estimated size of the galaxy is substantial, indicating a large and relatively massive system.
