The galaxy presents a largely smooth, elliptical morphology. Its light profile is concentrated towards the center, indicating a prominent galactic bulge. The color is predominantly yellow-orange, suggesting an older stellar population with lower rates of star formation. There is a slight asymmetry to the galaxy's overall shape, though there are no apparent signs of recent major mergers or tidal disturbances. The galaxy exhibits minimal internal structure, and it lacks discernible spiral arms or a distinct disk component. It appears to be a relatively isolated galaxy.
