The galaxy presents a somewhat amorphous morphology. It has a dominant, centrally concentrated bulge-like structure, exhibiting a yellow-white color. The concentration of light appears relatively smooth and centrally condensed. The presence of a fainter, distinct luminous region slightly offset from the main concentration is observed. This could be indicative of a minor interaction or merger event. There are potential traces of faint disk-like features. The overall color suggests an older stellar population.
