The galaxy presents a generally smooth morphology, appearing largely featureless in this observation. It exhibits an elliptical shape, displaying an intermediate roundness, with a slight elongation along one axis. The core of the galaxy appears to be a concentrated, bright region, likely dominated by older stellar populations. The color gradient suggests a shift from bluer hues in the outer regions, potentially indicating ongoing or recent star formation, to redder tones in the central bulge. There are no obvious signs of major mergers or significant tidal disturbances, although a slight asymmetry may suggest minor interaction or internal dynamic processes. The estimated physical size appears relatively compact for a galaxy at its redshift, suggesting it may be an early-type galaxy or a compact spiral galaxy.
