This galaxy appears to be an edge-on spiral galaxy. The disk is oriented almost perfectly along our line of sight, presenting a flattened, elongated profile. A prominent central bulge is visible, exhibiting a smooth, rounded morphology. This bulge displays a yellowish-white color, suggestive of an older stellar population. Fainter, diffuse light extends from the bulge along the galactic plane, indicating the presence of a stellar disk. The disk appears relatively smooth, with no obvious signs of strong spiral arm structures or distinct dust lanes. The galaxy exhibits a subtle color gradient, transitioning from the yellowish core to a bluer hue in the outer regions of the disk. This color shift is consistent with ongoing star formation in the outer regions of the galaxy, although the rate of star formation is likely low. Overall, the galaxy displays a regular structure, showing no clear evidence of recent major mergers or tidal disturbances. Minor irregularities or faint plumes may be present, but are not readily discernible.
