The galaxy appears as a disk galaxy with an estimated apparent size of approximately 14 arcseconds. The overall structure is somewhat disturbed. I see no distinct bulge, which suggests that it may be a late-type spiral galaxy. The spiral arms seem ill-defined, possibly exhibiting evidence of tidal disturbances. There are areas of blue luminosity indicating recent star formation, although limited. Based on my observations, a merger seems likely. There appears to be a notable color variation suggesting inhomogeneous stellar populations or patchy dust obscuration. It exhibits characteristics of both an undisturbed galaxy and also showing signs of merging, so it is hard to say what exactly is happening here. 
