The galaxy presents as a lenticular, disk-shaped structure oriented approximately edge-on relative to our line of sight. It exhibits a smooth, moderately elongated morphology, with no discernible spiral arms or prominent features such as dust lanes. The central bulge appears proportionally small, but distinct and bright, with a subtle colour gradient indicating a higher concentration of older stellar populations towards the nucleus. The colour of the galaxy is on the redder side, suggesting that it has likely ceased forming stars. There is no evidence of ongoing major mergers or significant tidal disturbances in this image, hinting at a relatively quiescent evolutionary history.
