The galaxy presents as a largely smooth and symmetrical object. It appears approximately circular in shape. The central region exhibits a high degree of luminosity, indicating a concentrated distribution of stellar populations or possibly an active galactic nucleus. There is a gradual decrease in surface brightness from the core outwards. The color appears generally yellowish-white. There is very little structural detail discernible at this resolution. A small part of the galaxy is disturbed, possibly merging with another galaxy.
