The observed galaxy appears to be a spiral galaxy, characterized by a disk-like structure with prominent spiral arms. It is not seen edge-on. Two clear arms emanate from the central region. These arms are loosely wound. There does not appear to be a strong central bar structure. The bulge is neither dominant nor insignificant in size, appearing moderate. The color suggests a relatively high rate of star formation with regions of blue interspersed between yellow. There is a close proximity between the main galaxy and a smaller galaxy. The separation between the center of the main galaxy and the satellite galaxy appears relatively small. There might be some minor disturbance in the structure of the larger galaxy, but nothing obvious.
