The galaxy presents a slightly elliptical morphology, suggestive of a disk galaxy viewed at a moderate inclination. There is a bulge, however, there are no notable spiral arm structures visible in the image. The light distribution appears relatively smooth and consistent, indicating the absence of prominent star-forming regions. The light emitted appears bluer in the core, and redder in the periphery, meaning there could be some dust around the outside of the galaxy. There is some evidence of a possible minor tidal disturbance. There is also a possibility of a merger event happening in this galaxy. 
