The galaxy appears to be a relatively smooth object, exhibiting a primarily elliptical morphology with a high degree of central concentration. Its overall color is indicative of an older stellar population, suggesting a diminished rate of ongoing star formation. The galaxy's light profile shows a gradual decline in brightness from the core outwards, consistent with a structure dominated by evolved stars. There is a hint of some disturbance. There is also a possible interaction between the body of the galaxy and a companion galaxy.
