This galaxy appears to be a spiral galaxy viewed at an oblique angle, possibly close to edge-on. A central bulge is visible, appearing a yellowish-orange hue, suggesting an older stellar population. The disk surrounding the bulge is somewhat faint and appears bluish-white, indicating the presence of younger, hotter stars. No distinct spiral arm structure is readily discernible, perhaps due to the viewing angle or the galaxy's morphology. There is a slight asymmetry to the disk, with one side appearing subtly more extended or disturbed. There does not appear to be any clear evidence of a major merger or tidal interaction, but some minor disturbance is possible. The galaxy appears relatively smooth in its overall structure, suggesting a lack of significant ongoing star formation.
