The galaxy presents as a relatively smooth, disk-shaped structure seen at a steep inclination, near edge-on from our line of sight. A central bulge is visible, appearing yellowish in color, suggesting an older stellar population. The disk exhibits a subtle color gradient, shifting towards bluer hues as it extends outward from the bulge. This color variation hints at ongoing star formation within the disk. No prominent spiral arm structure is discernible; however, slight irregularities in the disk's light distribution may indicate the presence of subtle or disrupted spiral features. Overall the galaxy displays a moderate luminosity. There is no clear evidence of major merging activity or significant tidal disturbances.
