The galaxy appears as a centrally concentrated object, exhibiting a largely smooth morphology. There is a hint of some features, potentially spiral arms or disturbances, though these are not sharply defined. The galaxy's color profile suggests a moderate level of ongoing star formation activity. The roundness of the galaxy indicates that it is not a highly inclined spiral galaxy. The apparent lack of strong tidal features suggests that it has not undergone a major merger recently, although there may be evidence of a minor disturbance. The overall luminosity suggests a galaxy of intermediate mass.
