The galaxy appears to be an elliptical or lenticular type, with a generally smooth, centrally concentrated light distribution. It exhibits a golden hue, suggesting an older stellar population. The galaxy displays a round morphology, with no obvious spiral arm structures, bars, or prominent dust lanes visible in this image. There is some asymmetry to the outer edges, possibly indicating a minor interaction with another galaxy or a past merger event. It's fairly luminous and large in size, indicating that it's a relatively massive galaxy. The color suggests low ongoing star formation. There is a slight disruption to the smooth light distribution, which could mean the galaxy is undergoing a minor disturbance, perhaps a merger. A tidal tail or other evidence of a major interaction is not visible in the image.
