The galaxy presents as a relatively smooth, bright object, with a mostly elliptical morphology. There is evidence of a potential interaction or merger event. The galaxy appears to have at least two distinct nuclei, with the primary nucleus being significantly brighter and more concentrated. The overall color is yellowish-orange, suggestive of an older stellar population with relatively little ongoing star formation, consistent with its round, smooth appearance. The fainter nucleus suggests a possible minor disturbance or merging event in its recent history. It is plausible that the galaxy is in the late stages of a merger, where tidal features might be too faint to observe in this image.
