The galaxy presents as a centrally concentrated, ellipsoidal structure with a smooth, diffuse light profile. It exhibits a predominantly yellow-orange hue, suggesting an older stellar population with lower rates of current star formation. There is a slight suggestion of a faint, diffuse halo extending beyond the main body of the galaxy, but no distinct spiral arms or prominent dust lanes are visible. The overall appearance is consistent with an elliptical or lenticular galaxy morphology, with minimal evidence of recent merger activity or significant star formation.
