The galaxy appears to be a spiral galaxy observed nearly edge-on. A central bulge component is visible, exhibiting a reddish hue. This likely indicates an older stellar population within the bulge. The galactic disk appears elongated and relatively thin, with a faint, bluish color that becomes more pronounced away from the central bulge. This color suggests the presence of younger, hotter stars in the disk, indicative of ongoing star formation. The galaxy does not appear to show any strong signs of recent major merger events.
