The galaxy presents as a centrally concentrated object with a relatively smooth profile. The core region exhibits high luminosity, appearing nearly uniform in color and brightness. Surrounding this bright central area is an extended, somewhat flattened disk. There is a slight hint of some disturbance or faint arms extending out from the central region. There are no obvious spiral arms or bar-like structures visible. The galaxy has a slight blue tint. The overall morphology suggests that it is not a late-stage spiral galaxy nor an elliptical galaxy. It could possibly be a lenticular galaxy or an early type spiral that has undergone some type of merging event. The blue color suggests the presence of younger stars.
