The galaxy presents as an edge-on spiral system. It exhibits a prominent central bulge that appears somewhat elongated along the major axis of the galaxy. The disk is viewed almost perfectly edge-on, obscuring any spiral arm structure. There appears to be a significant dust lane that bisects the galaxy along its central plane, contributing to the attenuation of light from the far side of the disk. The overall color profile suggests a relatively evolved stellar population, indicated by the reddish hue, particularly concentrated in the bulge. The lack of distinct blue regions suggests minimal ongoing star formation within the visible portion of the galaxy. The galaxy appears to be relatively isolated, with no obvious signs of interaction with nearby galaxies, though higher resolution imaging would be required to confirm this.
