This galaxy presents as a spiral type, viewed at an angle that is neither perfectly face-on nor edge-on. The spiral arms are evident, although not sharply defined, and appear somewhat tightly wound towards the central bulge. The bulge itself is prominent but not overly dominant in size relative to the overall disk.  A bar structure is potentially present but difficult to ascertain conclusively from the image. There are hints of disturbances in the disk possibly indicating a past or ongoing minor interaction with another galaxy. There also appear to be at least 2 possible nuclei. The galaxy's color is a mix of blue and red, suggesting a combination of both younger and older stellar populations with active star formation occurring within the spiral arms. The galaxy is resolved, allowing for detailed morphological analysis, and it has an average size.
