The galaxy presents as a single, concentrated object with a smooth and rounded morphology. The dominant color is a yellowish-orange hue, suggesting a stellar population that is relatively old and evolved, with lower levels of ongoing star formation. There is no apparent disk structure or spiral arms. The light is centrally concentrated. The galaxy appears relatively isolated, with no immediately obvious signs of major tidal disturbance or ongoing merger activity. Its estimated size indicates that it is a medium to large sized galaxy.