The galaxy presents as an edge-on disk galaxy. The central bulge is prominent and appears to be elliptical in shape. It exhibits a yellowish hue, suggesting an older stellar population. The disk component is elongated, and appears thin relative to the bulge. The overall color gradient suggests potential dust lanes within the disk, though they are not distinctly resolved. There are hints of disk features, but the image resolution limits detailed analysis. No significant signs of tidal disturbances or ongoing major mergers are immediately apparent. The galaxy's relatively smooth appearance indicates a potentially evolved system with a moderate star formation rate.
