The galaxy presents as a somewhat diffuse object. Its overall morphology appears largely smooth, with a slight elongation. The galaxy seems to have a primarily round shape. There are some minor disturbances to its structure, but these do not represent a merging event. The center of the galaxy is brighter than the surrounding areas. There is a hint of bluer light around the edges of the galaxy, indicating potential regions of star formation. The bulk of the galaxy is redder in color, perhaps indicative of an older stellar population.
