The galaxy presents an elliptical morphology, viewed nearly edge-on. A prominent dust lane bisects the galaxy along its major axis, appearing as a dark, reddish band. The galactic bulge is not distinctly visible, with the light profile increasing evenly to the center of the galaxy. The halo appears smooth and diffused, showing no evidence of spiral arms or star-forming regions. The colour profile suggests a redder population of stars, especially in the disk, indicating an older stellar population. The overall structure suggests the galaxy is potentially undergoing minor gravitational interaction, with the possibility of tidal disturbance evidenced by irregularities in the smooth light distribution in the outer regions.
