The galaxy presents as a disk galaxy, tilted at a high inclination relative to our line of sight. The disk exhibits a moderate degree of rotational symmetry. There appears to be a central bulge, although it is not highly pronounced. The light distribution suggests a relatively smooth, featureless morphology, with some indication of dust lanes along the plane of the disk, with minimal star forming regions.

The galaxy appears to have undergone no merging event. The outer regions appear to fade gradually with no distinctive features. The color index shows a dominance of redder wavelengths, indicative of an older stellar population, and possible dust obscuration.
