The galaxy presents as a spiral galaxy viewed at a relatively high inclination. The central bulge appears moderately sized and exhibits a yellowish hue, suggesting an older stellar population. The disk demonstrates some evidence of spiral arm structure, although the features are somewhat indistinct. The outer regions of the disk display bluer colors, possibly indicative of ongoing star formation. There are no prominent signs of a strong bar or any major merging activity; it looks relatively undisturbed.
