The galaxy presents as an elliptical, disk-shaped structure with a smooth, diffuse appearance. It exhibits a notable color gradient, transitioning from a yellowish-white core to a bluish-white outer region. The central bulge appears dominant and concentrated, indicating a higher stellar density. The galaxy shows a slight tilt relative to the observer's line of sight. There is no clearly visible spiral arm structure or dust lane features. The overall shape is somewhat elongated, with a relatively high axis ratio. Given the morphological characteristics, it is likely a disk galaxy with a prominent bulge, and a moderate amount of star formation activity.
