The galaxy presents as a single, largely featureless object. Its morphology appears predominantly smooth, with a high degree of roundness. There is little evidence of spiral arms or a distinct disk structure. It is slightly elongated. The color gradient suggests it is redder towards the core, possibly indicating an older stellar population concentrated there. There are no readily visible signs of on-going major mergers or significant tidal disturbances. Subtle asymmetry could indicate minor interaction or internal dynamical processes. The light emitted from the galaxy is typical of a large, relatively quiescent galaxy at a moderate redshift.
