The galaxy presents as a centrally concentrated system with a generally smooth appearance. It exhibits a slight elongation, though not strongly barred or spiral in nature. The color profile suggests a dominant older stellar population, indicated by the yellowish central bulge. Fainter blue-green hues are observed in a patchy ring further from the center, possibly indicating areas of more recent star formation. There is a nearby, smaller object that is reddish in color, potentially a satellite galaxy or another interacting component. The main galaxy shows only minor signs of disturbance. It appears to be in a relatively stable configuration.
