The galaxy appears to be an elliptical type with a prominent central bulge. Its overall shape is smooth and somewhat elongated. There is evidence of possible minor disturbances to the surrounding light distribution. The color profile shows a brighter core with a bluer outer rim and redder edges. There is a possible merger occuring with a smaller body that is impacting the distribution of light in the galactic disk. There is also a plume of stellar material being ejected from one end of the galaxy.