The galaxy appears to be a spiral type, presenting an inclined disk structure relative to our line of sight. The central bulge exhibits a yellowish hue, indicative of an older stellar population. The disk shows bluer regions interspersed with the yellow, suggesting ongoing star formation. The spiral arms are somewhat flocculent, lacking a grand design. There is some dust obscuration visible, particularly along the equatorial plane of the disk. No apparent signs of a major merger are seen, although some minor tidal features could be present.
