The galaxy appears as a relatively compact object with a concentrated central region. The morphology suggests a primarily smooth appearance, with a slight indication of underlying structure. The overall shape is approximately circular. There are hints of possible minor disturbances in the outer regions, with a slight asymmetry in its shape. Color gradients indicate a population with a redder hue, suggesting an older stellar population. The galaxy does not appear to be undergoing a major merging event, but there is a possible sign of minor interaction. 
