The galaxy appears to be a relatively smooth, elongated system, likely a disk galaxy viewed at a significant inclination. The central region exhibits a pronounced bulge, characterized by a yellow/orange hue, suggesting an older stellar population dominating this area. This region is relatively concentrated, but it appears smooth rather than showing the tightly wound spiral structure that might be expected in such a galaxy.

Surrounding the bulge is a fainter, bluish disk. The blue color indicates the presence of younger, hotter stars. The disk is not uniformly colored, showing hints of patchy areas within the blueish halo. The overall morphology hints at a galaxy undergoing relatively little current star formation. There is no strong evidence of a major ongoing merger, though some minor tidal disturbances cannot be completely ruled out given the slight irregularities in the outer regions of the disk.
