The galaxy presents as a relatively well-defined spiral structure. Two prominent spiral arms are discernible, loosely wound around a central bulge. The bulge appears moderate in size, not dominating the overall galactic disk. The disk exhibits a blue hue, suggestive of ongoing star formation activity within the spiral arms. The overall shape suggests a galaxy not viewed perfectly face-on, with a slight inclination relative to our line of sight. There is no obvious evidence of a strong bar structure bisecting the galaxy, nor any significant signs of major mergers or tidal disturbances. The galaxy appears relatively undisturbed, indicative of a system evolving in isolation. The presence of finer structural details are however hard to determine due to the resolution of the image.
