The galaxy presents as an elongated, cigar-shaped structure, viewed at a significant inclination. The central region exhibits a bright, concentrated core, suggestive of an older stellar population. Moving outwards from the core, a fainter, more diffuse disk is visible, appearing relatively smooth with a possible hint of spiral arm structure. There are no apparent signs of major ongoing mergers or significant tidal disturbances. The light distribution indicates a generally evolved system, potentially with a low rate of star formation. The overall morphology appears more elliptical than spiral, although a disky component cannot be ruled out.
