The galaxy presents as a somewhat elongated, intermediate system, neither perfectly elliptical nor a well-defined spiral. A central bulge region exhibits a concentrated luminosity, appearing nearly spheroidal and smooth in texture. The surrounding disk, if present, is only subtly defined; a faint blue hue suggests the presence of some star formation, although it appears to be at a relatively low rate. Some degree of disturbance is present. It is classified as a galaxy with a mass between 10^9 and 10^10 solar masses.
