The galaxy presents as a relatively smooth, concentrated object with an elliptical morphology. Its light profile appears centrally concentrated, indicating a significant bulge component, with color gradients showing an older stellar population dominating the core region. The disk component, if present, contributes less to the overall light. The galaxy is a yellowish-white color with slightly redder stars throughout, but it also has hints of blueish arms. There is no major or minor merging activity nor any disturbances, and its color and smooth appearance would suggest that it has a medium mass and moderate star formation rate.