The galaxy appears to be a relatively compact object with a generally smooth morphology. There is a bright central bulge, which appears somewhat elliptical in shape. This core exhibits a yellowish-orange hue, suggestive of an older stellar population. 

To one side, there is a distinct region of bluer light, indicating the presence of younger, hotter stars or active star formation. The galaxy shows signs of some sort of disturbance, with the blue region being somewhat separate from the main body. It is possible this galaxy is undergoing a merger event.

Overall, the galaxy is reasonably bright.
