The galaxy presents as a largely smooth, elliptical structure. It exhibits a concentrated central bulge, which appears to be the brightest region. The color gradient shifts from a yellow-white core to a redder outer halo. There are no readily discernible spiral arms or significant dust lanes. The overall morphology suggests a relatively evolved system, potentially an elliptical galaxy with little ongoing star formation. There is no visible evidence of any major mergers or tidal disturbances.
