The galaxy presents as a slightly disturbed system, exhibiting a notable degree of smoothness overall, with a relatively concentrated central region. The morphological characteristics suggest that the galaxy is in a state of interaction or recent merger activity, showing some minor disturbances.

The color indices suggest a well evolved population of stars. It appears relatively compact with a diameter of approximately 10 kpc, which is about half the size of our Milky Way. The distribution of light indicates the system is likely dominated by an elliptical component. The overall light profile indicates that the galaxy has largely ceased significant star formation.
