The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile. The color indices suggest a relatively old stellar population, with a redder hue dominating the overall appearance. There is minimal evidence of spiral arm structure or significant dust lanes. The galaxy's shape appears to be approximately in between round and cigar-shaped. A possible slight tidal disturbance is present, however this galaxy does not appear to be undergoing a major merger. Based on its apparent size and redshift, the galaxy is a moderate-sized galaxy with an estimated mass of approximately 10^11 solar masses. The galaxy's star formation rate is relatively low, suggesting that it is in the process of, or has recently completed, quenching its star formation activity.
