The galaxy appears as a fairly smooth object with an overall elliptical morphology. It has a concentrated central bulge that exhibits a yellowish hue, suggesting a population of older stars. A fainter, slightly bluer and elongated disk-like structure surrounds the bulge. There is a hint of some structure in the disk with possibly a minor disturbance to the overall shape. The disk appears relatively less prominent compared to the bulge, indicating that this is likely an early-type spiral or lenticular galaxy. The color gradient from the bulge to the outer regions suggests a decreasing stellar age, implying a possible ongoing, but low level of star formation within the disk. No pronounced spiral arm structures or significant dust lanes are readily apparent.
