The galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated light distribution. It has an overall color that is slightly red, which could be attributed to an older stellar population with lower levels of star formation activity, which is supported by green color found in the galaxy's disk. The morphology is predominantly spheroidal, with a somewhat elongated appearance, not perfectly circular. The galaxy does not show any signs of major disturbances or merging events based on the observed morphology. There may be some activity in the disk, but in general it exhibits low star formation relative to its mass. The galaxy appears to be relatively massive based on its size and overall luminosity.
