This galaxy exhibits a disk morphology, though it is not perfectly face-on. There is likely a central bulge component. The colors indicate ongoing star formation. The bluer hues present in the disk suggest the presence of younger, hotter stars, while the central regions appear redder, possibly indicating an older stellar population. There appears to be some minor disturbance in the galaxy's structure, but it appears generally undisturbed. The object displays a magnitude implying it is a large galaxy with an intermediate rate of star formation.
