The galaxy presents as an object with a central bulge, characterized by a smooth, diffused light profile, suggesting an older stellar population. Surrounding the central bulge is a fainter, less defined disk. The disk exhibits some structural irregularity, but not to the point of being heavily disrupted. The colors within this galaxy suggest a redder core and comparatively bluer outskirts. The redder core implies the presence of older, cooler stars. The bluer regions imply the presence of younger, hotter stars.
