The galaxy presents as a relatively smooth, centrally concentrated structure with a slight elongation. The color distribution is not uniform; a significant portion of the galaxy appears yellowish, while a more localized region exhibits a bluish hue. The overall morphology suggests a galaxy that is primarily smooth, yet may be experiencing or have recently experienced some form of interaction or internal process that has triggered localized star formation. Evidence of a merger is present. The galaxy displays signs of past or current interaction, potentially with another galaxy not visible in the image or a less significant merger event. Further investigation is warranted to determine the precise nature of these disturbances and their impact on the galaxy's overall evolution.
