The galaxy presents as an edge-on spiral, exhibiting a high degree of inclination relative to our line of sight. The disk component is prominent, displaying a relatively smooth texture. Some disturbances are likely minor. The bulge is observed to be rounded. Color gradients are present, with the central bulge appearing more yellow, potentially indicative of an older stellar population, and the outer disk exhibiting a bluer hue, possibly due to ongoing star formation. The galaxy displays no strong evidence of a major merger event.
