The galaxy appears to be an elliptical galaxy, potentially with a smooth morphology. The light distribution is centrally concentrated and appears to fade gradually toward the outskirts with an observed radius of approximately 2.6 kpc. The central region exhibits a yellowish hue, possibly indicative of an older stellar population. There are no prominent spiral arms or dust lanes visible. A slight redness is seen in the outer halo, further supporting an older, less active stellar population. There is no significant morphological disturbance observed, suggesting it is not currently undergoing a major merger. 
