The galaxy presents as a disk galaxy, observed edge-on from our vantage point. Its morphology suggests a relatively high inclination. The central bulge region is prominent, exhibiting a yellowish hue, which may indicate an older stellar population. The disk appears somewhat featureless, lacking obvious spiral arm structures or distinct dust lanes. Fainter bluish halos extend from the disk and may indicate recent and ongoing star formation. The overall structure appears undisturbed, suggesting a lack of recent major merger events. There is no obvious sign of tidal tails or stellar streams.
