The galaxy presents a somewhat irregular morphology, appearing neither purely elliptical nor a well-defined spiral. There is evidence of a slight disk-like structure, but it is not strongly pronounced. The galaxy is relatively compact, displaying a smooth central bulge. The color gradient suggests a higher concentration of older stellar populations. Some minor disturbance or interactions is present, perhaps due to minor tidal interactions. There is some suggestion of minor tidal features, faint extensions or asymmetries, which warrants further investigation into possible ongoing or past merger events.
