The galaxy presents an elliptical morphology, appearing largely smooth with a concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. The galaxy exhibits an elongated shape, though not extremely so, leaning towards a more spheroidal structure. There is faint bluer emission noticeable in the outskirts on one side. There may be some signs of minor tidal disturbances, but the galaxy is largely undisturbed and non-merging.