The galaxy presents a complex morphology, appearing as an apparent merger or interacting system. The primary component exhibits a relatively smooth, centralized luminosity profile, suggesting an elliptical or lenticular galaxy. This core region displays a dominant yellowish-orange hue, indicative of an older stellar population with minimal ongoing star formation. 

Adjacent to this primary component, there are noticeable irregular features, possibly tidal tails or disrupted spiral arms, which show bluer colors indicative of more recent star formation. These features extend outwards from the main body, disrupting the overall symmetry. The tidal features appear to be interacting with a smaller, bluer component, which could be a smaller galaxy actively merging or interacting with the larger one. The system is relatively compact.
