The galaxy presents as a generally smooth, elliptical structure with a high degree of central concentration. It appears nearly edge-on, exhibiting a distinct major axis. The core exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluer emissions are observed in the outer regions, potentially indicating the presence of younger stars or star forming regions, though these areas appear minimal. There is no visual evidence of spiral arms or a prominent disk. The galaxy lacks significant dust lanes or morphological disturbances, implying that it is not undergoing any major mergers or interactions with other galaxies. Its overall morphology is consistent with an elliptical galaxy with a centrally concentrated light profile.
