This galaxy exhibits characteristics suggesting an ongoing or recent merger event. Morphologically, it appears disturbed, displaying a notable asymmetry in its overall shape. A significant fraction of its light is concentrated in a bright, compact, blue-hued region, indicating a potential site of active star formation. This bluer region is juxtaposed against a more diffuse, yellowish component, possibly indicative of an older stellar population and/or dust obscuration. The general profile of the galaxy lacks a well-defined disk or spiral arm structure. The observed characteristics imply this system is not a quiescent, well-established elliptical or spiral galaxy but is dynamically active, likely due to gravitational interactions with another galaxy.
