The galaxy presents as a relatively smooth, rounded object with a concentrated central bulge. There is evidence of a slight colour gradient, shifting from a yellow-white core to a bluish halo or disk-like structure. The light distribution suggests an elliptical morphology, lacking prominent spiral arms or other distinct features. The lack of significant irregularities or tidal tails indicates it is likely not undergoing a major merger event. The roundness suggests that this galaxy is approximately spherical rather than highly flattened. Overall, the characteristics point towards a quiescent galaxy with a well-established stellar population and minimal ongoing star formation. 
