The galaxy presents an elliptical morphology with a smooth light distribution. It has a notable yellowish-orange hue, suggesting an older stellar population and a lower rate of ongoing star formation. There appears to be a second, smaller concentration of light located close to the brighter central area. There is evidence of a possible interaction or merger event, which could explain the disruption to the smoothness of the overall structure, but this is speculative and would need to be confirmed with more extensive observations. The galaxy exhibits an apparent magnitude suggesting it is moderately luminous. There is slight asymmetry in the color distribution.
