The galaxy appears to be a disk galaxy viewed at an oblique angle, exhibiting a flattened, elliptical shape. The central region displays a bright, concentrated luminosity, suggesting the presence of a galactic nucleus. Surrounding this core is a less-defined, diffuse region, potentially indicative of a stellar disk. There appears to be some evidence of a disturbance to the disk, as there is an irregular shape to its outer edges. Furthermore, the presence of blue light suggests ongoing star formation. The redder light on the periphery may indicate an older stellar population in the outer regions of the galaxy.
