The galaxy presents a mostly smooth morphology, appearing largely spheroidal. A slight elongation is detectable, but the overall form is well-rounded.  There is evidence of a bulge. The galaxy's light profile is centrally concentrated. Color gradients suggest some ongoing star formation activity, with bluer regions possibly indicating younger stellar populations.  No prominent spiral arms or disk structures are discernible from this image. There may be a minor disturbance or an early stage merger occurring.
