The galaxy appears as a small, faint disk, observed nearly edge-on. There is a central bulge which appears smoothly rounded, with an apparent lack of significant features within the disk itself. No strong dust lanes are visible. The galaxy exhibits a redder color, particularly in the central bulge region, suggesting an older stellar population and a low rate of ongoing star formation. The overall morphology suggests it may be a relatively evolved spiral galaxy, with no apparent signs of recent or ongoing major mergers, though perhaps minor disturbances may exist.
