The galaxy presents as a somewhat elliptical, yellowish-orange, moderately concentrated light source. The overall form appears relatively smooth, lacking prominent spiral arms or a distinct disk. The galaxy exhibits a slight elongation, suggesting a prolate spheroidal shape rather than a perfectly circular form. There is a faint, reddish hue observed in patches around the galaxy, potentially indicative of star-forming regions or dust. The galaxy shows no obvious signs of tidal disturbances or major mergers, although a very slight asymmetry cannot be entirely ruled out. Overall, it is consistent with a massive galaxy that may be undergoing a transition away from active star formation.
