The object appears to be a disk galaxy, oriented nearly edge-on from our perspective. The disk exhibits a relatively smooth, elongated structure. A central bulge is visible, with a concentration of light toward the center of the galaxy. The bulge appears somewhat rounded. No significant signs of active galactic nuclei activity or intense star formation regions are readily apparent. The dust lane is faintly visible. Based on the image, there is no strong evidence of any ongoing major merging activity or significant tidal distortions affecting the overall morphology.
