The galaxy appears to be an elliptical galaxy, with a smooth, diffuse light distribution. It exhibits a relatively high degree of symmetry. There is no obvious presence of spiral arms or prominent dust lanes. The galaxy appears to be lenticular, but difficult to precisely measure given the image quality. The color suggests an older stellar population, with a bias toward redder wavelengths. There is no apparent nuclear activity or unusual morphological features indicative of a recent merger event. The galaxy shows signs of being in the process of evolving into a red and dead state.
