The galaxy appears to be a relatively compact object with a moderate apparent size. Its overall morphology is somewhat smooth and elliptical in shape, but not perfectly so. There is some indication of mild disturbances or asymmetries in the galaxy's structure, possibly suggesting a past or ongoing interaction or minor merger.

The central region of the galaxy exhibits a slightly higher concentration of light. While there is a degree of smoothness, closer examination suggests that it does not have the characteristic features of a spiral galaxy. There appears to be at least one merger occurring.
