The galaxy presents as a relatively smooth, centrally concentrated object, suggesting an elliptical or lenticular morphology. It exhibits a moderate degree of roundness, appearing neither perfectly spherical nor highly elongated. The core is luminous, indicating a significant concentration of stars or potentially an active galactic nucleus, though no distinct features like spiral arms or a prominent bar are visible. There are no obvious signs of ongoing major mergers or significant tidal disturbances, however, there is a possibility of minor disturbances or a previous merger as the outer edges are irregular. Color gradients suggest some variations in stellar populations, although the overall color is red, which may indicate an older stellar population and relatively low levels of current star formation. The galaxy's apparent size is relatively small, indicating it is a distant object.
