The galaxy presents as a relatively smooth, elliptical morphology. It appears to be a lenticular galaxy, exhibiting a centrally concentrated bulge that fades into a disk structure without prominent spiral arms. There is minimal evidence of star formation, indicated by a lack of bright blue regions associated with young, massive stars. The central bulge emits a yellowish light, consistent with an older stellar population. The outer regions of the galaxy are fainter and bluer than the core, but not markedly so. It may have recently undergone a minor disturbance or merging event, but appears to be in a relatively relaxed state.
