The galaxy appears to be a disk galaxy, exhibiting a flattened, elliptical morphology. Its central bulge presents a concentrated, yellowish-white light, suggesting an older stellar population. A fainter, more diffuse disk surrounds the bulge, with a noticeable tilt relative to our line of sight. The disk shows a bluer hue, hinting at the presence of younger, hotter stars and potential ongoing star formation. There is some asymmetry observed in the disk's outer regions, along with hints of faint spiral arms, suggesting possible gravitational interactions or past merger events. The overall structure seems relatively smooth, implying that the galaxy has not undergone a recent major merger. The galaxy displays a significant amount of red light and dust extinction, indicating that the galaxy may be more massive than it looks.
