The galaxy presents a generally smooth and somewhat elongated morphology, showing characteristics that appear to be somewhere between round and cigar-shaped. A dominant central bulge is visible with an extended, diffuse halo surrounding it. There seems to be evidence of either a minor interaction or internal disturbances within the galaxy, and signs of merging and tidal forces. The presence of both blue and red regions suggests there is a mix of both younger, star-forming regions and older stellar populations.
