The galaxy appears as a moderately bright, somewhat elongated object. It exhibits a dominant central bulge. There is a suggestion of a disk-like structure. The light distribution is relatively smooth across the galaxy, without obvious strong features. There may be an ongoing merger event occurring, as hinted by some visual disturbance of the main galaxy body. Alternatively, these could be artifacts. The estimated size of the galaxy is fairly typical, and has a reasonable mass. It shows a fairly high, but normal, rate of star formation. It is primarily intermediate in color.
