The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light distribution. It has a dominant central bulge, characterized by a high concentration of older stars, indicated by the yellowish-orange hue. The galaxy appears somewhat elongated in shape, with the overall structure lacking prominent spiral arms or distinct features. There are signs of minor disturbances. Overall, it is a relatively luminous galaxy, indicative of a substantial stellar population and ongoing star formation.
