The galaxy presents as a slightly elongated, disk-shaped object, observed at an angle that provides a nearly face-on view. The central bulge appears moderately defined. There are no well defined spiral arms; the galaxy is smooth in overall appearance, but not completely featureless. There is some indication of internal structure, possibly related to minor disturbances or faint spiral patterns. The color distribution within the galaxy suggests a potential mix of stellar populations. A slightly bluer hue is evident in the disk relative to the inner regions, indicating ongoing star formation. The outer regions fade gradually, and there is no obvious tidal debris or interaction with neighboring objects. Overall, the galaxy appears to be relatively quiescent, potentially a transitioning type between disk galaxies and lenticular galaxies.
