The galaxy appears to be a disk galaxy, viewed edge-on from our perspective. A prominent dust lane is bisecting the galaxy, obscuring the central bulge region. This dust lane appears relatively thick and uniform across the visible span of the galaxy. The central bulge exhibits a yellowish hue, suggestive of an older stellar population. The galactic disk outside of the central bulge seems to show a greenish tint, possibly indicating some on-going star formation. The galaxy does not appear to exhibit any strong tidal features or signs of recent major merger activity, suggesting it has a relatively relaxed morphology. The galaxy has a generally flattened shape with no obvious signs of strong spiral arms. The overall structure appears relatively smooth, with a notable central concentration.
