This galaxy exhibits characteristics of a disk galaxy viewed at an oblique angle. It has a bright, concentrated central bulge, likely composed of older stars. The bulge exhibits a yellowish hue. Extending outward from the bulge is a fainter, flattened disk. There is some asymmetry visible in the disk structure, with hints of spiral arm segments on one side. The color distribution across the disk suggests regions of ongoing star formation, indicated by the presence of bluer and reddish hues in various regions of the arms. Overall, the galaxy appears relatively undisturbed, with no obvious signs of recent major merger events.
