The galaxy presents a predominantly smooth morphology, with a centrally concentrated bulge that appears nearly spherical. The color profile suggests an older stellar population dominating the bulge, indicated by its yellowish hue. Surrounding the bulge, there is a subtle, diffuse disk component. The disk region shows some evidence of structure and potential star formation as seen by subtle variations in color. Overall, the galaxy exhibits characteristics consistent with a disk galaxy undergoing an intermediate level of star formation. A faint tidal feature is visible at the bottom. It shows a hint of ongoing interaction, although a significant merger is unlikely.
