The galaxy presents a primarily smooth morphology, with a prominent central bulge and a more diffuse surrounding disk. The overall shape is somewhat elongated, appearing as an ellipse.

Color gradients are visible across the galaxy. The central region exhibits a strong yellowish hue, suggesting an older stellar population. Moving outward from the center, the color gradually shifts toward a slightly bluer tone, particularly noticeable in certain regions of the disk. This bluer tint potentially indicates the presence of younger, hotter stars, and perhaps ongoing star formation in those areas.

There is no indication of major tidal disturbances or ongoing mergers. The galaxy appears relatively undisturbed, with a fairly regular structure.
