The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. Its overall shape is largely round, with a slight deviation towards an intermediate form, lacking a prominent disk structure. There is a slight hint of disturbance. The galaxy's color profile shows a concentration of light towards the redder end of the spectrum, indicating an older stellar population, with very minimal ongoing star formation. The galaxy appears moderately massive, suggesting it has undergone substantial evolution.
