The galaxy exhibits a generally elliptical morphology, appearing moderately smooth with some indication of disturbed features, possibly suggesting an ongoing or recent merger event. The core region shows a concentration of light, transitioning to a fainter halo. Color gradients suggest a higher concentration of older stellar populations within the core, trending towards younger stars in the outer regions, with the center being more red in color and the halo being more green in color. The estimated size is roughly 5.2 kiloparsecs in radius. There appear to be disturbances of material leaving the galaxy, indicating a possible outflow. The overall appearance and color profile are consistent with a galaxy having a stellar mass in the approximate range of 10^9 solar masses.
