The galaxy presents as an elongated, edge-on spiral. A prominent central bulge is visible, exhibiting a reddish-yellow hue, suggesting a population of older stars. The disk appears thin and extended, with hints of blueish light emanating from regions along the galactic plane, possibly indicating areas of active star formation. There appears to be little to no evidence of tidal features or major disturbances, suggesting it is not currently undergoing a major merging event, though there is evidence of minor disturbance in its morphology. The bulge appears to be more rounded than boxy. The galaxy does not have a smooth appearance; it has disk-like morphology.
