The galaxy presents a largely smooth, rounded morphology, indicative of an early-type system. There is a subtle color gradient visible, with the central region appearing slightly more yellow and the outer regions exhibiting a bluer hue. There are no readily apparent spiral arms or a prominent disk-like structure. Faint, diffuse light extends outwards from the central region, suggesting a gradual decline in stellar density. No signs of significant tidal disturbances or ongoing merger events are visible, which supports the smooth classification. The overall appearance points to a relatively relaxed galaxy, potentially an elliptical or S0 type, that has largely exhausted its gas supply and has a low star formation rate.
