The galaxy presents as a moderately bright, relatively smooth object with a discernible central bulge. Its shape is approximately round, though not perfectly spherical. The light distribution appears generally uniform, with a slight concentration towards the core, indicating a possible elliptical morphology. There are some subtle hints of features or a disk-like component, but it is difficult to confirm with certainty due to the resolution. There is no major or minor distortion of the galaxy. It exhibits no clear signs of a recent or ongoing major merger event, although the light distribution suggests some degree of disturbance. Color gradients suggest a slightly older stellar population, with a moderate amount of recent star formation.
