The galaxy presents as a generally smooth, elliptical morphology. There is a bright, concentrated central bulge that transitions gradually into a diffuse halo. Color gradients indicate an older stellar population, with the central regions exhibiting a yellowish-orange hue, suggestive of evolved stars. There is no strong evidence of distinct spiral arms or significant dust lanes. The galaxy's overall form is relatively rounded, with a slight elongation. There are no obvious signs of major mergers or tidal disturbances. The apparent size suggests a moderately large galaxy at its given redshift. Star formation rate appears to be subdued, or perhaps concentrated within the central regions and obscured by dust. The overall impression is that of a galaxy that is dominated by an older stellar population and has undergone significant evolution.
