This galaxy appears as a moderately bright, elliptical-like structure. It presents a relatively smooth appearance, with a central bulge that transitions gradually into the outer regions. The color profile indicates an older stellar population, with a dominant yellowish-orange hue in the central region. There is evidence of some bluer components in the outer disk regions. This may indicate more recent, ongoing, or past star formation. The shape appears somewhat elongated. There is no strong evidence of spiral arms or a well-defined disk, although it could be obscured by the relatively high redshift or poor resolution of the image. The galaxy does not obviously show signs of active merging, though some asymmetry could suggest a minor interaction in its past. Overall, the galaxy appears as an evolved system with a likely substantial mass and moderate star formation.
