The galaxy presents an elliptical morphology, appearing generally smooth and lacking distinct spiral arms. The central bulge exhibits a bright, concentrated luminosity, indicative of a high stellar density, possibly an actively feeding supermassive black hole. The outer regions fade gradually into the background, without any clear truncation of the stellar halo. Color gradients appear minimal, suggesting a relatively homogenous stellar population. There is a slight elongation, deviating from a perfect circle. I do not see any signs of merging activity.