The galaxy presents a well-defined spiral structure. Evident spiral arms extend outwards from a central bulge. These arms appear relatively tightly wound and exhibit a non-uniform distribution of light, suggesting regions of active star formation. The central bulge displays a yellow hue, indicative of an older stellar population. There is some evidence of ongoing or recent interaction events given the irregular morphology; possible tidal features or distortions may be present. The galaxy shows a moderate inclination with respect to our line of sight, neither face-on nor edge-on, which gives a good view of its spiral structure. The disk component appears to be the most dominant component in terms of size and the galaxy has no strong bar structure.
