The galaxy appears to be an elliptical galaxy or a lenticular galaxy viewed at a slight angle. Its central bulge is prominent and appears smooth with a yellow-orange hue, potentially indicating an older stellar population. There is a faint indication of a disc-like structure extending beyond the bulge, but it lacks defined spiral arms. The overall shape is elongated, with a cigar-like appearance. There is a possible minor disturbance observed on one side, but the galaxy generally appears undisturbed with a smooth morphology. The galaxy appears relatively massive, likely consisting of over 100 billion solar masses. The galaxy exhibits a relatively low star formation rate, suggesting it is towards the end of its stellar life cycle.
