The galaxy appears to be a spiral galaxy, seen at an oblique angle. The central bulge is prominent and has a smooth, yellowish hue, suggesting an older stellar population. The disk shows faint spiral arm structure. The arms are slightly bluer than the bulge, which implies the presence of younger, hotter stars and ongoing star formation. There may be evidence of a weak tidal feature or minor disturbance, but it is not definitive. Overall, the galaxy appears relatively undisturbed and not undergoing a major merger. The light distribution suggests a relatively high mass. The moderate blue color indicates an intermediate star formation rate.
