The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. It exhibits a generally rounded shape with a slight deviation towards an intermediate form. There is a possible indication of a faint disk. The galaxy's color profile suggests a population of older stars and a relatively low star formation rate, although some ongoing star formation is also possible. The object does not appear to be undergoing a major merger, but some minor disturbance may be present. Overall, the galaxy appears to be a relatively undisturbed system.
