The galaxy appears to be an elliptical type. It exhibits a largely smooth and concentrated light profile with a round morphology. There is a small concentration of light close to the center of the galaxy that could potentially be a sign of an on-going or recent merger. The color distribution is largely homogenous across the galaxy, presenting with yellow/orange hues indicative of an older stellar population. There are no distinct spiral arms or dust lanes visible, which is consistent with an elliptical classification.
