The galaxy appears to be a disk galaxy, seen at an oblique angle. Its morphology is generally smooth with a bright central bulge, likely composed of older stellar populations, giving it a yellowish hue. The disk is elongated, exhibiting an elliptical shape, suggesting it is not viewed face-on. There is a subtle color gradient from the center outwards, with the outer regions displaying a slightly bluer tint, potentially indicating the presence of younger, hotter stars within the disk. There is no clear evidence of spiral arm structure, though the limited resolution may obscure such features. There are no obvious signs of major disturbances or ongoing mergers with other galaxies, however, a slight lopsidedness may indicate a minor tidal interaction or past merger event. Overall, the galaxy appears to be relatively evolved and quiescent.
