The galaxy appears as a centrally concentrated, relatively smooth object. Its overall shape is elliptical, with a high degree of roundness. The color gradient suggests a possible lack of significant ongoing star formation. The core region exhibits a yellowish hue, potentially indicating an older stellar population. There are no obvious signs of spiral arms or a prominent disk structure. There is no evidence of any major merging events or tidal distortions. The galaxy's apparent size is small, but it is likely a distant object.
