The galaxy presents as a somewhat smooth and centrally concentrated object. Its morphology appears elliptical or lenticular, exhibiting a relatively high degree of roundness. The central bulge region is bright, appearing yellow, suggesting an older stellar population. A fainter blue disk surrounds the bulge. The color indicates a younger stellar population, implying ongoing star formation. There are no indications of strong spiral arm structures or a bar. There is a slight asymmetry in the outer regions of the disk, potentially suggesting a minor gravitational disturbance, like a tidal interaction with a smaller galaxy, but this is not obviously a merging event.
