The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and rounded morphology. It appears relatively undisturbed, with no obvious signs of a major merger event, although a minor disturbance cannot be ruled out. The galaxy exhibits a concentrated central bulge with a moderately luminous core region and is likely a mature system with a relatively high mass. The light profile suggests an older stellar population, visible by its yellowish color, with a possible indication of ongoing, albeit moderate, star formation activity. There are no clearly defined spiral arms. Overall the galaxy appears to be a rather typical example of its type and appears quite symmetrical in form.
