The galaxy appears to be a relatively smooth elliptical. There is a concentration of luminosity towards the center, exhibiting a bright core that fades into the outer regions. The color profile suggests a population of older stars, more concentrated towards the core. The galaxy exhibits a slight elongation, its shape is roughly in between round and cigar-shaped. There does not appear to be any major disturbances to the morphology of the galaxy, indicating that it is not currently undergoing a major merging event. There may be a minor disturbance of the disk but this is difficult to see.
