The galaxy appears to be a relatively large, luminous system. It exhibits a moderately elliptical morphology, displaying a dominant bulge component. The overall color profile suggests an older stellar population, with a noticeable concentration of light towards the central region. There is faint evidence of a disk structure but it is hard to distinguish. The galaxy's light profile appears smooth, with no prominent spiral arms or dust lanes visible. Weak, distorted structure is observed on the outskirts of the galaxy. Based on these observations, this galaxy can be classified as an early-type galaxy, likely an elliptical or lenticular type.
