The galaxy presents as a concentrated, centrally brightened object. Its morphology appears largely smooth, with a dominant spheroid component. The color profile suggests a relatively evolved stellar population. The galaxy exhibits a slightly elliptical shape, with the absence of prominent spiral arms or other disk-like features. There are no readily apparent signs of major mergers or significant tidal disturbances. Overall, the galaxy appears to be an early-type system, potentially an elliptical or lenticular galaxy, residing at a considerable cosmological distance.
