The galaxy presents as a barred spiral, oriented approximately edge-on from our perspective. A central bulge is prominent, exhibiting a smooth, concentrated distribution of light suggesting an older stellar population. The disk component is well-defined and demonstrates the presence of spiral arms, although their exact number is indeterminate. The spiral arms appear tightly wound, indicating a relatively high shear rate within the disk. There is no evidence of significant tidal distortions or ongoing mergers, although a minor interaction with a smaller object cannot be entirely ruled out based on visual inspection alone. The overall color is consistent with a galaxy undergoing relatively low levels of star formation.
