This galaxy exhibits a complex morphology. It is somewhat diffuse, appearing relatively smooth, but displays subtle, non-uniform features. The overall light distribution seems concentrated, yet the edges lack a well-defined boundary. There is some evidence of a spiral structure, but it is faint and disturbed, likely with minor disturbance, or possibly more significant interaction with another galaxy. There may be merging activity occurring, the result is unclear. It has a magnitude indicative of moderate brightness within the observed field. The galaxy's color is indicative of an older stellar population.
