The galaxy appears to be an elliptical type, exhibiting a generally smooth, concentrated light profile. Its color is predominantly yellow-orange, suggesting a population of older stars and a relatively low rate of current star formation. The galaxy appears mostly symmetrical with only a slight degree of elongation. There is a minor disturbance visible in the galaxy's morphology, indicative of a possible interaction or past merger event. There is an object that is located close to the galaxy, but whether or not they are physically bound is difficult to determine from this image. 
