The galaxy presents a predominantly smooth and centralized morphology. It is elliptical or perhaps a lenticular galaxy seen nearly face-on. The light distribution suggests a relatively uniform stellar population, though with some very slight color variation from the core outwards. The central region exhibits a bright yellowish-white hue, potentially indicative of an older stellar population. There appears to be minimal presence of dust lanes or active star-forming regions. Any faint spiral arms that might exist appear tightly wound and indistinct. Overall, the galaxy appears to be relatively isolated and undisturbed.
