The galaxy presents as an edge-on or nearly edge-on disk galaxy. A prominent dust lane is visible, bisecting the galaxy along its major axis. The bulge appears rounded, with a concentrated luminosity toward the center. Evidence of a faint, extended disk is noted, but the limited resolution of the image prevents detailed analysis of any spiral structure. There does not appear to be any signs of current interaction with other galaxies in the immediate field. Based on the color profile there appears to be ongoing star formation within the galaxy.
