The galaxy presents an elliptical morphology, appearing largely smooth and concentrated. The light profile suggests a dominant bulge component with a high degree of central concentration. Color gradients are subtle, with a slightly redder hue towards the center, potentially indicative of an older stellar population. There is a slight irregularity in the overall shape, as if it were a disturbed system. Evident tidal features are absent, though a subtle asymmetry may suggest minor ongoing or past interaction. Star formation appears to be largely quiescent, with no prominent HII regions visible. The galaxy displays a moderate redshift, placing it at a substantial cosmological distance. It possesses a considerable mass, typical for galaxies of its type and luminosity.
