The galaxy presents a morphology indicative of a disk galaxy, though seen at a near edge-on angle. The central bulge appears prominent and moderately sized, exhibiting a yellowish hue suggesting an older stellar population. The disk component shows a generally smooth texture, with faint, diffuse features hinting at spiral arm structures. A bar feature bisecting the bulge is subtly discernible. Overall, the galaxy does not show any strong signs of recent mergers or major disturbances, although minor asymmetries in the disk's outer regions may indicate past gravitational interactions. The bluer colors in the outer disk regions show more recent star formation has occurred in these areas. The galaxy's reddish-brown color suggests that star formation has slowed.
