Observed galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. The light distribution suggests a generally spheroidal shape, showing a high degree of symmetry, though not perfectly round. There is a lack of any discernible spiral arm structure or dust lanes. The galaxy appears to be a yellowish-orange hue, indicating an older stellar population. The central region exhibits higher surface brightness compared to the outer regions. Some minor disturbances seem to exist at the periphery. Overall, the galaxy exhibits characteristics indicative of a relatively evolved system.
