The galaxy appears to be a spiral galaxy observed at an angle, suggesting a disk-like structure. It appears as a moderately bright object with a generally smooth texture, though there is some indication of internal structure. The central region shows a concentration of light, likely the galactic bulge. Faint features extend from either side of this central bulge; these may be spiral arms. It is likely that star formation is present, though at low levels, given the reddish coloration within the arms. The disk is moderately inclined, and the color profile of the galaxy appears redder than the surrounding field. The overall morphology suggests a galaxy that is relatively undisturbed, though there are some subtle asymmetries in the disk shape. 
