The galaxy presents as a likely spiral or lenticular system at an intermediate redshift. It exhibits a bright central bulge, suggestive of an older stellar population, with an estimated effective radius of approximately 3.4 kpc. Its red-sequence color indicates relatively low levels of on-going star formation. Overall morphology indicates a system that is primarily smooth, showing a minimal distortion due to recent mergers or interactions. Its shape is elliptical and mostly disk-like, not being a completely round sphere or very elongated cigar. Evidences suggest no major merging events, but a minor disturbance is possibly observed.
