The galaxy appears to be a relatively compact, elliptical or lenticular galaxy at intermediate redshift. It presents with a generally smooth, diffuse light distribution, lacking prominent spiral arms or a distinct central bulge. The galaxy exhibits a color gradient, with a slightly bluer hue in its outer regions compared to the more yellow-red central region. This could indicate the presence of a younger stellar population in the outer disk. The galaxy’s overall morphology is somewhat elongated, suggesting a possible elliptical shape or a disk seen at an angle. There are no apparent signs of major mergers or significant tidal disturbances, though subtle asymmetries could indicate minor interactions. The overall color suggests a relatively evolved stellar population, consistent with a moderate level of star formation activity.
