The galaxy presents a largely smooth morphology with a central, bright concentration of light. The overall shape is approximately elliptical, though not perfectly round, appearing somewhat elongated. There is little evidence of prominent spiral arms or significant disk-like structure. A gradual decrease in light intensity extends outwards from the core. Faint, diffuse features surround the core, but they do not exhibit any sharp edges or distinct substructures that would indicate an ongoing major merger event. There is no clear visual evidence of active star formation regions; the overall color suggests an older stellar population and minimal dust obscuration.
