The galaxy presents as an elliptical morphology, appearing largely featureless and smooth. The light profile exhibits a concentrated central bulge, diminishing in intensity towards the outer edges. The color gradient suggests a predominantly older stellar population, with a yellow-orange hue dominating the core region, indicative of evolved stars. There is no clear evidence of spiral arm structures or significant dust lanes. The galaxy displays a slight elongation, deviating marginally from a perfectly circular form. There are no apparent signs of recent or ongoing major merger events or tidal distortions, although a very slight asymmetry may indicate minor gravitational interactions in its past or present. Given its redshift, the galaxy appears relatively compact in angular size, suggesting a considerable distance. Considering the apparent magnitude and estimated redshift, this is likely a fairly luminous galaxy. The observed color profile, along with the smooth morphology, points to low levels of star formation activity.
