The galaxy appears as a faint, elongated structure, possibly a spiral galaxy viewed at a significant angle. A central bulge is present, displaying a yellowish hue, suggestive of an older stellar population. Fainter, bluish arms extend from the central region, indicating regions of more recent star formation. The overall morphology is somewhat disturbed, possibly indicative of a minor interaction or merger event, which could explain the regions of more recent star formation. The galaxy is relatively small and compact. A diffuse halo is not clearly distinguishable, given the apparent faintness and the limited resolution of the image.
