The object appears to be an elliptical galaxy at an approximate redshift of 0.036. The light is concentrated toward the center, suggesting an older stellar population. The galaxy appears largely spheroidal and smooth in shape, showing little evidence of spiral arms or significant disk-like features. There may be a hint of tidal disturbance or minor asymmetry in the outer regions, but the galaxy is generally undisturbed. The object has a stellar mass in the range of approximately 10^9 solar masses and low star formation rates.
