The galaxy presents as a relatively small, disk-shaped system, observed nearly edge-on from our vantage point. The morphology suggests a spiral galaxy, although detailed spiral arm structure is not discernible in this image, implying they are tightly wound, or obscured. The central bulge is prominent and exhibits a smooth, rounded appearance. The bulge is noticeably brighter than the rest of the disk, with a color profile tending towards redder wavelengths, suggesting an older stellar population. The disk appears relatively thin and uniform in color, trending towards red, but not quite as red as the bulge. There is no immediately obvious evidence of active star formation regions or significant dust lanes within the observed disk. There are no strong signs of recent or ongoing mergers or tidal disturbances in the immediate vicinity, however more information would be needed to confirm this finding.
