The galaxy presents a generally smooth morphology, with a dominant central bulge. Its overall shape appears to be somewhere between round and elliptical. The galaxy exhibits a color gradient, transitioning from a yellowish-orange core to a slightly bluer outer region, suggesting potential variations in stellar populations and star formation activity. There is no clear evidence of spiral arms or a well-defined disk. There is no obvious signs of ongoing or recent major merger events or tidal disturbances.
