The galaxy presents as a somewhat elliptical object, exhibiting a central bulge with a diffuse, extended halo. The core is bright and slightly blue-shifted, suggesting the presence of a population of hot, young stars or possibly an active galactic nucleus. There are some disturbances within the structure of the galaxy. This is likely due to ongoing interactions with another galaxy. The disturbance appears to be a minor one. The overall color of the galaxy indicates a mix of stellar populations, with evidence of both ongoing star formation and an older, redder population.
