The galaxy presents as a centrally concentrated object with an overall smooth appearance. Its morphology suggests a relatively evolved system. There is subtle evidence of a disk-like structure, although the smoothness indicates that the spiral arms are likely tightly wound, or the disk may be more lenticular in nature. The color gradient suggests a population of older stars dominates, with a weaker component of younger, bluer stars. There is no obvious evidence of a major ongoing merger or strong tidal interaction with another galaxy, although minor disturbances cannot be ruled out. The galaxy appears to be fairly round and there is no significant elongation or asymmetry visible.
