The galaxy appears to be an elliptical galaxy, characterized by a smooth, featureless morphology and a high degree of central concentration. It exhibits a roughly round shape, with a slight elongation that may indicate the presence of a weak disk component, or a minor disturbance in the morphology. The color profile indicates older stellar populations, with a reddish hue suggesting a lower rate of recent star formation. No distinct spiral arms or bar structures are discernible. Based on the observed color gradient, this galaxy is a massive galaxy with lower star formation than most other galaxies. There is no signs of tidal tails or obvious merging signatures, which indicate that this galaxy is most likely in a relatively relaxed state with some minor merging.