The galaxy appears to be an elliptical type. It exhibits a generally smooth morphology without prominent spiral arms or dust lanes. The light is concentrated towards the center, indicating a significant bulge component. The shape is moderately elongated, but not significantly cigar-shaped. There is no obvious evidence of a major ongoing merger, though a minor disturbance cannot be ruled out based on this image alone. The color is generally yellowish, suggestive of an older stellar population.
