The galaxy presents as a relatively smooth and rounded object, exhibiting a general elliptical morphology. There is a slight elongation, but the aspect ratio does not suggest a highly flattened disk. The galaxy appears to be a dominant galaxy. There is no evidence of major mergers or significant tidal disturbances. The color is consistent with an older stellar population, with a redder hue, indicative of less active star formation. It has a small size on the image, suggesting it is an older, more evolved galaxy with a substantial stellar mass.
