The galaxy presents a distinct spiral morphology, though the angle of inclination obscures a face-on view. The spiral arms are relatively tightly wound. A prominent central bulge is observed, exhibiting a yellowish-white hue, suggesting an older stellar population. The arms display a bluer coloration, indicative of ongoing star formation. The disk appears relatively smooth, with only minor disturbances observed. Dust lanes are present, particularly near the central bulge. Based on the color and morphology, this is likely a relatively massive galaxy with moderate star formation activity.
