The galaxy presents as a relatively smooth, centrally concentrated object. Its shape is generally round. There is a slight elongation observable, although the dominant impression is of circular symmetry. The galaxy exhibits a yellowish hue, suggestive of an older stellar population. There is no clear evidence of spiral arms or a distinct disk structure. No obvious signs of an active galactic nucleus or ongoing major star formation regions are visible. There may be some minor disturbance. Overall, the galaxy appears to be an elliptical or lenticular type, lacking significant features.
