The galaxy presents as a centrally concentrated, luminous structure with a relatively smooth appearance. The light profile appears to transition gradually from a bright, nearly unresolved core to fainter outer regions. There is an overall elliptical morphology, appearing more elongated than perfectly circular, with no distinct spiral arm structure or prominent features like dust lanes visible. There are subtle irregularities or disturbances to the structure, suggesting possible minor gravitational interaction with another galaxy. There is a hint of blue color, indicating the presence of some young, hot stars, but redder hues dominate.