The galaxy presents as a spiral type, observed at an angle between face-on and inclined. A central bulge is visible, exhibiting a yellowish hue, potentially indicative of an older stellar population within. Extending from the bulge are discernible spiral arms, appearing somewhat tightly wound, giving the galaxy a flocculent nature. The arms display a mottled blue color, suggesting regions of active star formation. There are hints of dust lanes interweaving through the spiral arms, especially on one side of the galaxy. Overall, the galaxy appears to be a relatively isolated spiral, without apparent signs of major mergers or significant tidal disturbances.
