The galaxy appears to be a spiral galaxy, with a central bulge that exhibits a yellowish hue, suggesting a population of older stars. The disk appears to have spiral arms, although they are not well-defined and appear somewhat flocculent. The color is bluer towards the outer regions of the disk, which is consistent with ongoing star formation. The galaxy appears to be moderately inclined to our line of sight. There might be a minor disturbance in the morphology, possibly indicative of a past or ongoing interaction. Overall, the galaxy seems to be in a relatively late stage of evolution, with a mix of both old and young stellar populations.
