The galaxy presents a predominantly smooth morphology, suggesting it is likely an elliptical galaxy or a lenticular galaxy with a significant bulge component. It appears relatively round in shape. There is no clear evidence of spiral arms or a well-defined disk. The central region exhibits a brighter, more concentrated luminosity, indicative of a galactic nucleus or a dense stellar population. Surrounding the central region, there is a more diffuse, extended halo or envelope of stars, with a slight colour gradient suggesting varying stellar populations or dust content. Overall, there is no apparent signs of major disturbances such as tidal tails or strong asymmetries, possibly indicating the absence of ongoing major merger events. There may be a slight disturbance.
