The galaxy presents as a smooth, elongated, spindle-shaped object. Its structure is primarily amorphous, lacking readily discernible spiral arms or a prominent central bulge. The light distribution suggests a relatively even stellar population throughout the galaxy's body. The color gradient indicates a possible redder core, though the resolution is insufficient for definitive identification. The galaxy appears largely undisturbed, with no obvious signs of recent mergers or tidal interactions. The absence of strong blue light suggests a subdued star formation rate. The object's overall morphology points towards an elliptical galaxy.
