The galaxy presents a largely smooth morphology, with little evidence of distinct spiral arms or a prominent central bulge. It appears elliptical or lenticular in shape, exhibiting a high degree of radial symmetry. The color profile suggests a redder population, potentially indicating an older stellar population with diminished recent star formation. There is no noticeable dust lane or significant morphological disturbance, which, combined with the smooth appearance, points towards a lack of major mergers.
