The galaxy appears to be a lenticular or early-type spiral, exhibiting a smooth, centrally concentrated bulge. There is some evidence of a faint disk component, but it appears largely featureless. The central bulge displays a yellowish hue, suggesting an older stellar population. The disk shows a bluer color, indicative of some recent or ongoing star formation, although it is not particularly prominent. There is a slight asymmetry in the disk's luminosity distribution, possibly a minor disturbance. Overall, the galaxy seems to be transitioning away from active star formation.
