The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology with a somewhat elliptical shape. The light distribution suggests a dominant bulge component, possibly indicative of an older stellar population. There is some subtle asymmetry with disturbances, potentially suggesting a merger event or interaction with a companion galaxy. The galaxy has a redder component, indicating an area of dust or an older population of stars. Overall the galaxy appears to be relatively quiescent in terms of star formation.
