This galaxy appears to be a spiral galaxy, viewed nearly edge-on. There is a central bulge that appears yellowish-orange, possibly indicating an older stellar population. The disk is relatively smooth, with subtle hints of dust lanes along its length and there is some evidence of younger, bluer stars in the outer regions of the disk. The galaxy is not obviously interacting with any other galaxies, although there are some minor irregularities that may indicate disturbances or a minor merger history. Overall, the galaxy seems to be relatively undisturbed and undergoing moderate levels of star formation. The overall morphology is consistent with a late-type spiral galaxy, though without more detailed spectra or higher resolution imaging, it is difficult to classify the galaxy with great accuracy.
