The galaxy presents a lenticular morphology with a smooth, diffuse light distribution. The central region appears brighter and more concentrated, exhibiting a yellowish hue, suggestive of an older stellar population. Extending outwards from the core is a fainter, blueish halo, potentially indicating more recent star formation. There are subtle indications of disturbed morphology in the outer regions, suggesting a possible past interaction. Overall, the galaxy appears to be an intermediate-mass system at a moderate redshift.
