The galaxy appears to be an elliptical type, exhibiting a generally smooth and rounded morphology. There's a concentration of light towards the center, suggesting a prominent galactic nucleus. The overall color is relatively uniform, leaning towards a slightly bluer hue in the outer regions and whiter towards the center. This indicates a mix of stellar populations, with possibly younger, bluer stars in the outskirts and older populations dominating the core. There is a slight indication of minor disturbance to the galaxy. The galaxy has a estimated diameter of approximately 5 kiloparsecs, and a mass range of approximately 9 billion to 12 billion solar masses. Based on its estimated star formation rate and specific star formation rate, this galaxy is most likely currently dormant.