The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a concentrated central bulge that transitions smoothly into a fainter, more diffuse halo. The galaxy displays a yellow-orange hue, suggesting an older stellar population with fewer young, hot stars. There is no apparent spiral structure or evidence of significant dust lanes. The overall morphology indicates that this galaxy is likely a mature system that has largely ceased active star formation. It shows no signs of major mergers or tidal disturbances, maintaining a generally undisturbed, round shape. The size of the galaxy is compact, suggesting a moderate physical extent for its redshift.
