The galaxy presents as a centrally concentrated, elliptical-like structure. The light distribution appears relatively smooth, with a noticeable lack of distinct spiral arms or well-defined features in this image. The core region exhibits a bright, concentrated luminosity, suggesting a high stellar density, likely an actively star forming region. The outer regions gradually fade, forming a diffuse halo. The overall color profile suggests a population of older stars, as indicated by the reddish hue, with possible younger, bluer populations in the core. There may be subtle hints of minor disturbances in the overall structure, or interactions occurring, but these are not obvious. Based on the redshift and absolute magnitude, this appears to be a massive galaxy with a relatively low star formation rate.
