The galaxy appears to be an elliptical or lenticular galaxy, with a primarily smooth morphology and a high degree of rotational symmetry. Its light distribution is concentrated towards the center and gradually diminishes outwards, without any obvious spiral arm structure or dust lanes. The lack of distinct features indicates a relatively quiescent state.

The color of the galaxy is predominantly yellowish-white, suggesting an older stellar population with fewer young, massive stars. The estimated size is a few kiloparsecs across. There is a subtle hint of blueish color at the periphery, perhaps indicating some low level of recent star formation in the outer regions of the disk. Some possible minor tidal interactions seem possible.
