The galaxy presents as a spiral type with a predominantly face-on orientation. It exhibits distinct spiral arm structures, though they appear somewhat flocculent rather than grand design. The central bulge is moderately sized and displays a yellowish hue, suggesting an older stellar population. The spiral arms themselves show a bluer color, indicative of ongoing star formation. A subtle, somewhat elongated structure potentially resembling a weak bar can be discerned within the central region. The disk appears relatively smooth with faint dust lanes running along the spiral arms. There is a noticeable lack of strong disturbances or signs of a major merger event. Overall, the galaxy appears to be a relatively isolated and unperturbed spiral.
