The galaxy presents with a generally smooth morphology. Its overall form appears to be elliptical in nature, though not perfectly spherical. The central region exhibits a bright, concentrated luminosity, suggesting the presence of a significant stellar population and potentially a central supermassive black hole. There is a slight elongation, hinting at a possible transition between an elliptical and lenticular classification. Subtle dust lanes are not discernible, but it cannot be definitively ruled out due to the image quality. There is a slight indication of minor disturbances in the outer regions. The overall light profile suggests that the galaxy is not undergoing a major merger event.
