The galaxy presents as a relatively smooth, elliptical morphology, appearing mostly round in shape. There is a clear central concentration of light, suggestive of a prominent bulge. The color appears generally red, potentially indicating an older stellar population with ongoing star formation. There is evidence of a secondary object in close proximity, which could indicate minor interaction or disturbance. No strong spiral arm structures are visible. Based on its appearance, the galaxy may be undergoing or have recently undergone a minor merger event.