The galaxy presents a largely smooth morphology, appearing as an elliptical type galaxy when analyzed via visual inspection. The central bulge is prominent and exhibits a yellowish hue, potentially indicating an older stellar population. Moving outward from the core, the galaxy’s light gradually diminishes. While generally smooth, there is a hint of a flattened structure, suggesting a possible disk component, though it is not sharply defined. There are no obvious signs of ongoing major merger activity, although a subtle asymmetry or minor disturbance cannot be entirely ruled out. The overall shape is mostly in-between round and elongated, closer to round. Star formation rate seems rather low.