The galaxy presents as a moderately luminous object at a redshift of approximately 0.24. It exhibits a generally smooth morphology, with a subtle but discernible disk-like structure. The color profile suggests a well-mixed stellar population with intermediate age stars, but there is still some recent star formation activity. There is no current evidence for any major ongoing merger events or significant tidal disturbances, though minor interactions cannot be ruled out. The galaxy appears somewhat rounded in shape, without significant elongation or distortion, consistent with a classification of elliptical or early-type spiral. The effective radius suggests a galaxy of considerable size.
