The galaxy presents as a relatively smooth, though not perfectly featureless, object. There is evidence of a disk-like structure, but it is not sharply defined; there is a diffuse, central bulge and a wider, more flattened component. The colour profile indicates a dominant population of older stars, with a general redder hue throughout the entirety of the structure. There might be some limited evidence of internal substructure or minor disturbances, but the overall form suggests the galaxy is mostly undisturbed. The high fraction of smoothly distributed light suggests it is a galaxy that is not currently undergoing a major merger. The rate of new stars forming is slow, and the overall morphology suggests it is a quiescent galaxy dominated by older stellar populations.
