The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light distribution without any prominent spiral arms or distinct features. The galaxy's color gradient suggests an older stellar population dominating the light output. There is a concentrated bright core, possibly indicating the presence of a supermassive black hole at the galactic center. There is a high degree of central light concentration that gradually fades out into the surrounding halo. There is no apparent ongoing star formation in the galaxy due to the absence of blue light. There are no signs of tidal disturbances or ongoing mergers. The galaxy appears to be a relatively isolated system, undisturbed by significant gravitational interactions.