The galaxy presents as a concentrated, centrally luminous object. It is approximately circular in shape, exhibiting a high degree of smoothness throughout its structure. Color gradients suggest an older stellar population dominating the core, with a gradual shift towards bluer colors in the outer regions. The relative smoothness implies a lack of significant ongoing mergers or tidal disturbances. The distribution of light suggests a possible elliptical morphology with a spheroidal component. The colors are indicative of moderate redshift. Star formation is likely suppressed in the core. Overall, the galaxy appears relatively isolated and undisturbed with a possible weak active galactic nuclei signature.
