The galaxy appears to be a relatively compact object, likely an elliptical or lenticular galaxy, given its generally smooth appearance. There is a subtle elongation, deviating slightly from a perfectly circular shape. Its color profile appears to be redder in the central region and bluer along the edges, suggesting an aging stellar population concentrated toward the core with some younger, bluer stars present in the outer regions. No distinct spiral arms or significant dust lanes are visible, but the slight irregularities in the outer halo suggest the possibility of a past minor merger event. A slight disturbance in the symmetry of the galaxy's halo indicates possible tidal interactions. Overall, the galaxy's structure implies a evolved system with minimal ongoing star formation and some evidence of past interactions.
