This galaxy appears to be a spiral galaxy viewed at a slight incline. It exhibits a bright, concentrated central bulge with a yellowish-white hue, indicating an older stellar population. The disk shows evidence of spiral arm structure, though the arms are somewhat tightly wound. There is a bluer color, especially in the outer regions of the disk, suggesting the presence of younger, hotter stars and ongoing star formation. The galaxy displays moderate dust lanes within the spiral arms, obscuring some of the starlight and contributing to a mottled appearance in the disk. Overall, the galaxy appears to be relatively well-defined with no signs of strong tidal disturbances.
