This galaxy appears to be an elliptical galaxy at a moderate redshift. The galaxy exhibits a generally smooth morphology, with a high degree of roundness to its shape. There is no indication of significant spiral arm structure or a prominent disk. The light distribution appears concentrated toward the center, gradually fading outward with no obvious signs of major disturbances or active galactic nuclei. The galaxy exhibits a color profile that shifts towards redder wavelengths, potentially indicating an older stellar population and a low rate of ongoing star formation. Evidence suggests a potential interaction or minor disturbance in the galaxy's form, but without any definitive strong signs of an active merger.
