The galaxy presents as a relatively luminous, disk-shaped structure viewed at an oblique angle. A central bulge exhibits a yellowish hue, possibly indicative of an older stellar population or dust obscuration. The disk displays a broader color gradient, transitioning from the yellow-dominant central region to bluish tones in the outer regions. The bluer color may suggest regions of more recent star formation. The disk appears relatively smooth. The overall shape is elongated, and the galaxy doesn't obviously show evidence of significant ongoing interaction or disruption by another galaxy. The general morphology appears consistent with an intermediate to late-type spiral galaxy, but without clear spiral arm structures easily discernible from the image.
