The galaxy appears as a flattened, elongated structure seen nearly edge-on. A prominent central bulge is visible, exhibiting a relatively smooth and concentrated light distribution suggesting an older stellar population. The disk component is thin and extends outwards from the bulge on either side, displaying a mottled texture indicative of dust lanes and potentially some regions of active star formation. The color gradient suggests that the bulge exhibits a yellowish-orange hue, while the disk appears bluer, consistent with a population of younger, hotter stars within the disk. No obvious spiral arm structure is discernible, likely due to the near edge-on viewing angle. There does not seem to be any indication of recent merger activity or major disturbances to the galaxy's overall structure, and the shape is relatively undisturbed.
