This galaxy presents as a spiral galaxy, displaying an orientation somewhat between face-on and edge-on relative to our line of sight. There is evidence of a flattened disk structure. A distinct, centrally located bulge is visible, exhibiting a yellowish hue suggestive of an older stellar population and/or dust obscuration. The disk shows a bluer color, perhaps indicating regions of more recent star formation. There are hints of spiral arm structure extending from the central bulge, though these features appear somewhat diffuse and flocculent, rather than well-defined. The overall morphology suggests ongoing, though perhaps not intensely vigorous, star formation activity within the disk component. Irregularities in the outer regions of the disk may be suggestive of minor gravitational interactions with neighboring galaxies, though a major ongoing merger event is not readily apparent.
