The galaxy appears as a singular, generally smooth structure with some notable colour variations. It presents with a somewhat elliptical morphology, leaning toward a rounded shape, but not perfectly spherical. 

The light distribution across the galaxy is not uniform. There is a brighter, more concentrated core region emitting light that is more white-shifted. Adjacent to this core is a distinct region that shows more of a red shift. This could be a redder, older stellar population.

Based on the slightly disturbed, blob-like nature of the galaxy, a prior or ongoing merger event cannot be ruled out, although the object appears to be mostly undisturbed. 
