The galaxy presents as a relatively smooth, elliptical or lenticular system. It exhibits a concentrated central bulge that is bright and yellow-orange in color, suggesting a population of older stars. The galaxy appears to be somewhat elongated, but without any prominent disk-like features or spiral arms visible in this image. There is no visible ongoing major merger activity. There may be a minor disturbance based on the light distribution, but nothing drastic. The galaxy shows a smooth profile, with no distinct knots of star formation that are readily apparent. The overall color and morphology imply a galaxy with a significant population of evolved stars and relatively low ongoing star formation, and the size of the half light radius seems on par with other galaxies at its redshift.
